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        <title>HGSS - recent papers</title>


    <link rel="self" href="https://hgss.copernicus.org/articles/"/>
    <id>https://hgss.copernicus.org/articles/</id>
    <updated>2026-08-13T11:58:18+02:00</updated>
    <author>
        <name>Copernicus Publications</name>
    </author>
        <entry>
            <id>https://doi.org/10.5194/hgss-2026-12</id>
            <title type="html">The Remarkable Scientist and Writer Ukichiro Nakaya and his "Black Moon" and "White Moon" Worlds
            </title>
            <link href="https://doi.org/10.5194/hgss-2026-12"/>
            <summary type="html">
                &lt;b&gt;The Remarkable Scientist and Writer Ukichiro Nakaya and his "Black Moon" and "White Moon" Worlds&lt;/b&gt;&lt;br&gt;
                Kevin Hamilton and Wataru Ohfuchi&lt;br&gt;
                    Hist. Geo Space. Sci. Discuss., doi:10.5194/hgss-2026-12,2026&lt;br&gt;
                    &lt;b&gt;Preprint under review for HGSS&lt;/b&gt; (discussion: open, 0 comments)&lt;br&gt;
                Ukichiro Nakaya (1900&amp;#8211;1962) was a Japanese scientist who created the first artificial snowflake in 1936 and figured out how temperature and humidity affect snow crystal shapes &amp;#8212; a result smmarized in the "Nakaya diagram." He studied ice in Greenland, wrote popular science essays for everyday readers (earning him the nickname "Japan's Carl Sagan"), and was a pioneer in making educational films. This article, written for his 125th birthday, covers his life, his science and his writing.
            </summary>
            <content type="html">
                &lt;b&gt;The Remarkable Scientist and Writer Ukichiro Nakaya and his "Black Moon" and "White Moon" Worlds&lt;/b&gt;&lt;br&gt;
                Kevin Hamilton and Wataru Ohfuchi&lt;br&gt;
                    Hist. Geo Space. Sci. Discuss., https://doi.org/10.5194/hgss-2026-12,2026&lt;br&gt;
                    &lt;b&gt;Preprint under review for HGSS&lt;/b&gt; (discussion: open, 0 comments)&lt;br&gt;
                The physicist Ukichiro Nakaya (1900&amp;#8211;1962) is renowned in Japan for his contributions to snow and ice science and for his outstanding achievements as a writer and film maker. His meticulous field observations and his laboratory investigations led to seminal discoveries about snow crystals. Notably in 1936 Nakaya produced the world&amp;#8217;s first artificial snow crystal created in a cloud chamber. This allowed him to determine the systematic dependence of snow crystal shapes on the conditions at formation, a result now summarized in the widely known &amp;#8220;Nakaya diagram&amp;#8221;. In the 1950&amp;#8217;s Nakaya began collaborations with the US Snow, Ice and Permafrost Research Establishment investigating the properties of glacial ice, notably including fieldwork in Greenland during the pioneering years of the deep ice coring project there. Nakaya was a very prolific writer of essays published in Japanese magazines, and his essays were often republished in book collections, many still in print today. His writing for the general public about science has led to his reputation as &amp;#8220;The Carl Sagan of Japan&amp;#8221;, but his writing extended more broadly to many areas of culture. Nakaya was also a pioneer in making educational documentary films and he was instrumental in the formation of a major film studio in Japan.</p&gt; <p>This article was initiated to mark Nakaya&amp;#8217;s 125th anniversary year and aims to introduce his life and achievements to a broad international audience. We review Nakaya&amp;#8217;s biography and highlights of his scientific career, and include some brief discussion of the Japanese cultural context for his scientific work. We recount some particularly dramatic aspects of Nakaya&amp;#8217;s life which was shadowed by the great historical developments of his era, notably the Second World War. We also review his contributions to Japanese literature of his time. We sample a handful of Nakaya&amp;#8217;s articles written for the general public in order to convey the scope and flavour of his literary <em>oeuvre</em>. We describe in detail two of Nakaya&amp;#8217;s most ambitious magazine essays: &amp;#8220;World of the Black Moon&amp;#8221; and &amp;#8220;World of the White Moon&amp;#8221;, which are of particular interest as vivid first person accounts of middle 20<sup>th</sup&gt; century research field trips (to Hawaii and Greenland, respectively). &amp;#8220;World of the White Moon&amp;#8221; is also notable for including a very early description for the general public of the issue of anthropogenic climate change.
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-08-13T11:58:18+02:00</published>
            <updated>2026-08-13T11:58:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-2026-9</id>
            <title type="html">George Perkins Merrill's Analyses of Chondrules and Chondritic Meteorites
            </title>
            <link href="https://doi.org/10.5194/hgss-2026-9"/>
            <summary type="html">
                &lt;b&gt;George Perkins Merrill's Analyses of Chondrules and Chondritic Meteorites&lt;/b&gt;&lt;br&gt;
                Carl N. Drummond&lt;br&gt;
                    Hist. Geo Space. Sci. Discuss., doi:10.5194/hgss-2026-9,2026&lt;br&gt;
                    &lt;b&gt;Preprint under review for HGSS&lt;/b&gt; (discussion: open, 1 comment)&lt;br&gt;
                George Perkins Merrill, a Smithsonian scientist in the early 1900s, made discoveries about meteorites that still shape our understanding of the solar system's birth. Using microscopes to examine tiny spherical grains called chondrules, the building blocks of stony meteorites, he concluded they formed through multiple processes.. He also showed that meteorites record a history of alteration by heat and pressure over time. His laid groundwork for meteorite research for over a century.
            </summary>
            <content type="html">
                &lt;b&gt;George Perkins Merrill's Analyses of Chondrules and Chondritic Meteorites&lt;/b&gt;&lt;br&gt;
                Carl N. Drummond&lt;br&gt;
                    Hist. Geo Space. Sci. Discuss., https://doi.org/10.5194/hgss-2026-9,2026&lt;br&gt;
                    &lt;b&gt;Preprint under review for HGSS&lt;/b&gt; (discussion: open, 1 comment)&lt;br&gt;
                George Perkins Merrill (1854&amp;#8211;1929) was the preeminent American meteoriticist of the first quarter of the 20<sup>th</sup&gt; Century. He applied to that science his pioneering knowledge and skill in the petrographic analysis of chondritic meteorites. Throughout his long and distinguished career with the United States National Museum, now the Smithsonian Institution of Washington, D.C., Merrill authored over seventy publications on meteorites. While many of those contributions described new irons and stones which had come into the museum&amp;#8217;s collection, a pair of papers concerning the origin of chondrules and the evidence for and causes of metamorphism of chondritic meteorites led directly to his selection as the second recipient of the J. Lawrence Smith Medal which was awarded by the National Academy of Sciences in 1922 for outstanding accomplishments in the study of meteorites. The origins, primary arguments, and subsequent reception of those two landmark papers are herein reviewed. Particular attention is given to how Merrill&amp;#8217;s hypotheses on chondrule formation and the evidence for thermal and dynamic metamorphic alteration of chondrites have come to underpin and advanced modern understandings of the early history of the solar system.
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-07-02T11:58:18+02:00</published>
            <updated>2026-07-02T11:58:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-2026-8</id>
            <title type="html">History of the Max-Planck-Institut f&#252;r Aeronomie and its scientific projects (1958&#8211;2004)
            </title>
            <link href="https://doi.org/10.5194/hgss-2026-8"/>
            <summary type="html">
                &lt;b&gt;History of the Max-Planck-Institut für Aeronomie and its scientific projects (1958–2004)&lt;/b&gt;&lt;br&gt;
                Kristian Schlegel&lt;br&gt;
                    Hist. Geo Space. Sci. Discuss., doi:10.5194/hgss-2026-8,2026&lt;br&gt;
                    &lt;b&gt;Revised manuscript accepted for HGSS&lt;/b&gt; (discussion: closed, 7 comments)&lt;br&gt;
                A detailed history of the Max-Planck-Institut f&amp;#252;r Aeronomie (MPAe), including its research and deleopment.
            </summary>
            <content type="html">
                &lt;b&gt;History of the Max-Planck-Institut für Aeronomie and its scientific projects (1958–2004)&lt;/b&gt;&lt;br&gt;
                Kristian Schlegel&lt;br&gt;
                    Hist. Geo Space. Sci. Discuss., https://doi.org/10.5194/hgss-2026-8,2026&lt;br&gt;
                    &lt;b&gt;Revised manuscript accepted for HGSS&lt;/b&gt; (discussion: closed, 7 comments)&lt;br&gt;
                The <em>Max-Planck-Institut f&amp;#252;r Aeronomie</em&gt; located in Katlenburg-Lindau, Germany, had a clearly defined beginning and end. It commenced on 1 January 1958 with the merging of the <em>Max-Planck- Institut f&amp;#252;r Ionosph&amp;#228;renforschung</em&gt; (ionospheric research) and the <em>Max-Planck-Institut f&amp;#252;r Physik der Stratosph&amp;#228;re</em&gt; (physics of the stratosphere), and it concluded in 2004 with the renaming in <em>Max-Planck-Institut f&amp;#252;r Sonnensystemforschung</em&gt; (solar system research &amp;#8211; MPS). This manuscript reviews the organization, scientific research, and development that took place over these 47 years.
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-25T11:58:18+02:00</published>
            <updated>2026-06-25T11:58:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-17-61-2026</id>
            <title type="html">Obituary: Bodo Reinisch (1936&#8211;2025)
            </title>
            <link href="https://doi.org/10.5194/hgss-17-61-2026"/>
            <summary type="html">
                &lt;b&gt;Obituary: Bodo Reinisch (1936–2025)&lt;/b&gt;&lt;br&gt;
                Dieter Bilitza&lt;br&gt;
                    Hist. Geo Space. Sci., 17, 61&#8211;63, https://doi.org/10.5194/hgss-17-61-2026, 2026&lt;br&gt;
                Obituary: Bodo Reinisch (1936-2025)
            </summary>
            <content type="html">
                &lt;b&gt;Obituary: Bodo Reinisch (1936–2025)&lt;/b&gt;&lt;br&gt;
                Dieter Bilitza&lt;br&gt;
                    Hist. Geo Space. Sci., 17, 61&#8211;63, https://doi.org/10.5194/hgss-17-61-2026, 2026&lt;br&gt;
                
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-22T11:58:18+02:00</published>
            <updated>2026-06-22T11:58:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-2026-2</id>
            <title type="html">Classical Antiquity Origin of Spatial Data Underlying Portolan Charts: How Pietro Vesconte Might Have Assembled the <em>Carta Riccardiana</em> Utilising Maps in Marinus of Tyre&#8217;s projection
            </title>
            <link href="https://doi.org/10.5194/hgss-2026-2"/>
            <summary type="html">
                &lt;b&gt;Classical Antiquity Origin of Spatial Data Underlying Portolan Charts: How Pietro Vesconte Might Have Assembled the Carta Riccardiana Utilising Maps in Marinus of Tyre’s projection&lt;/b&gt;&lt;br&gt;
                Tome Marelić&lt;br&gt;
                    Hist. Geo Space. Sci. Discuss., doi:10.5194/hgss-2026-2,2026&lt;br&gt;
                    &lt;b&gt;Revised manuscript accepted for HGSS&lt;/b&gt; (discussion: closed, 5 comments)&lt;br&gt;
                This manuscript provides the first-ever cartometric study of portolan chart geometry that firmly corroborates the classical antiquity origin of their spatial data. The conclusions are not solely based on the numerical approach, yet they are also substantially supported by the available historical records. Concurrently, it provides a detailed overview of the history of cartometric studies of portolan charts, especially in terms of explaining the benefits and constraints of their methodology.
            </summary>
            <content type="html">
                &lt;b&gt;Classical Antiquity Origin of Spatial Data Underlying Portolan Charts: How Pietro Vesconte Might Have Assembled the Carta Riccardiana Utilising Maps in Marinus of Tyre’s projection&lt;/b&gt;&lt;br&gt;
                Tome Marelić&lt;br&gt;
                    Hist. Geo Space. Sci. Discuss., https://doi.org/10.5194/hgss-2026-2,2026&lt;br&gt;
                    &lt;b&gt;Revised manuscript accepted for HGSS&lt;/b&gt; (discussion: closed, 5 comments)&lt;br&gt;
                The remarkably accurate representation of coastlines on late mediaeval portolan charts has garnered significant scholarly interest in uncovering the origin of their spatial data, with the prevailing hypothesis suggesting that they are authentic products of their time, created by synthesising numerous shipborne bearing and distance measurements. The pursuit of those answers also prompted the establishment and advancement of a cartometric approach, through which they can be attained with quantitative accuracy. This study is based on cartometric analyses and historical evidence, providing a comprehensive examination of the anonymous <em>Carta Riccardiana</em&gt; portolan chart, presumably created by Pietro Vesconte between 1300 and 1325. It posits a paradigm shift regarding the late mediaeval origin hypothesis, tangibly indicating that the conventional geometry of portolan charts was likely developed by late mediaeval copyist-cartographers who utilised regional maps from classical antiquity, originally made <em>in the projection of Marinus of Tyre</em&gt; calibrated to their mid-latitudes as inputs, which they partially scaled and gradually tilted, using a map in <em>Ptolemy&amp;#8217;s first projection</em&gt; as a reference model. Concurrently, the article provides a historical overview of the most significant cartometric studies in the field, critically analysing their unique systemic parameters that have influenced various hypotheses regarding the origin of portolan charts&amp;#8212;specifically, the systemically induced similarity with the modern map in the Mercator projection, which is, in the case of the <em>Carta Riccardiana</em>, at least, a misleading notion.
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-11T11:58:18+02:00</published>
            <updated>2026-05-11T11:58:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-17-37-2026</id>
            <title type="html">A 300-year history of understanding and classifying clouds, from a German language perspective
            </title>
            <link href="https://doi.org/10.5194/hgss-17-37-2026"/>
            <summary type="html">
                &lt;b&gt;A 300-year history of understanding and classifying clouds, from a German language perspective&lt;/b&gt;&lt;br&gt;
                Peter Winkler&lt;br&gt;
                    Hist. Geo Space. Sci., 17, 37&#8211;59, https://doi.org/10.5194/hgss-17-37-2026, 2026&lt;br&gt;
                Before the Enlightenment, clouds were described phenomenologically. The vacuum pump&amp;#8217;s invention enabled the formation of mist droplets by experiment, prompting questions about why clouds float. Around 1800, early proposals for cloud classification emerged. However, it wasn&amp;#8217;t until manned balloon ascents provided detailed atmospheric data that the physical basis of cloud formation became clear, even though accurately depicting clouds in atlases remained challenging for some decades.
            </summary>
            <content type="html">
                &lt;b&gt;A 300-year history of understanding and classifying clouds, from a German language perspective&lt;/b&gt;&lt;br&gt;
                Peter Winkler&lt;br&gt;
                    Hist. Geo Space. Sci., 17, 37&#8211;59, https://doi.org/10.5194/hgss-17-37-2026, 2026&lt;br&gt;
                <p>Otto von Guericke was the first who experimentally demonstrated cloud formation by expanding and cooling of compressed air before 1663. Scientists initially grappled with the very question of why clouds float. Early explanations were hampered by limited theory, imprecise instruments, and gaps in meteorological knowledge.</p&gt;        <p>First attempts for distinguishing various cloud types arose towards the end of the 18th century. A key turning point came in 1803 when Howard proposed a first systematic scheme using Latin terminology for different cloud types. This effort laid the cornerstone for what would evolve into today's internationally recognized cloud classification system. The path to accurate understanding was long and iterative; early laboratory work and imprecise instruments produced repeated misjudgements that endured for decades. Manned balloon ascents provided direct measurements of meteorological parameters in the free atmosphere and in clouds, but more reliable and bias-free instruments and advances in theory were necessary to achieve reliable results.</p&gt;        <p>Additional techniques had to be developed to determine cloud altitudes and track their motion, gaining knowledge of vertical temperature and moisture profiles that shape different cloud types. Beginning in the 1890s, large-scale movements in the upper atmosphere were recognised by coordinated international observations.</p&gt;        <p>Contemporary early cloud atlases were published despite the limitations of low-contrast, poor photographs. Alternatives, like paintings or cloud watercolours, were even used to overcome these early hurdles. Coordinated observations using daily pilot balloons, kites, and later weather aircraft allowed researchers to further explain cloud formation both in stable and unstable atmospheric conditions. In addition, stratospheric and mesospheric clouds were discovered.</p&gt;        <p>After many efforts to publish international and national cloud atlases the World Meteorological Organization's founding in 1951 enabled the first modern International Cloud Atlas in 1956, standardising cloud observation practices and nomenclature.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-04-02T11:58:18+02:00</published>
            <updated>2026-04-02T11:58:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-2026-6</id>
            <title type="html">The Fate of Y.S. Ma, China's First Female Geologist
            </title>
            <link href="https://doi.org/10.5194/hgss-2026-6"/>
            <summary type="html">
                &lt;b&gt;The Fate of Y.S. Ma, China's First Female Geologist&lt;/b&gt;&lt;br&gt;
                Jian Zhao Yin&lt;br&gt;
                    Hist. Geo Space. Sci. Discuss., doi:10.5194/hgss-2026-6,2026&lt;br&gt;
                    &lt;b&gt;Preprint under review for HGSS&lt;/b&gt; (discussion: final response, 5 comments)&lt;br&gt;
                In 1944, Ms. Y.S. Ma, the only female geologist in China at the time was killed at the age of 25. This year marks the 82nd anniversary of her tragic death. This article is dedicated to the young scholar who died before achieving her goal, leaving future generations deeply saddened.
            </summary>
            <content type="html">
                &lt;b&gt;The Fate of Y.S. Ma, China's First Female Geologist&lt;/b&gt;&lt;br&gt;
                Jian Zhao Yin&lt;br&gt;
                    Hist. Geo Space. Sci. Discuss., https://doi.org/10.5194/hgss-2026-6,2026&lt;br&gt;
                    &lt;b&gt;Preprint under review for HGSS&lt;/b&gt; (discussion: final response, 5 comments)&lt;br&gt;
                In April 1944 during the War of Resistance against Japan, three young scientists were killed by bandits in the field. Among the three were Ms. Y.S. Ma, the only female geologist in China at the time, a young geologist fluent in five foreign languages &amp;#8203;&amp;#8203;despite never having been abroad, and Mr. T.Y. Hsu and Mr. K. Chen, both budding and accomplished geologists. They were killed on the same day, at the ages of 25, 36, and 28 respectively. This year marks the 82nd anniversary of their tragic deaths. This article is dedicated to these three young scholars who died before achieving their goals, leaving future generations deeply saddened.
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-03-27T11:58:18+01:00</published>
            <updated>2026-03-27T11:58:18+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-17-25-2026</id>
            <title type="html">The founding actor of T&#252;rkiye's petroleum geology: Cevat Ey&#252;p Ta&#351;man and his legacy in the national energy policies
            </title>
            <link href="https://doi.org/10.5194/hgss-17-25-2026"/>
            <summary type="html">
                &lt;b&gt;The founding actor of Türkiye's petroleum geology: Cevat Eyüp Taşman and his legacy in the national energy policies&lt;/b&gt;&lt;br&gt;
                Oğuz Mülayim&lt;br&gt;
                    Hist. Geo Space. Sci., 17, 25&#8211;35, https://doi.org/10.5194/hgss-17-25-2026, 2026&lt;br&gt;
                <span data-olk-copy-source="MessageBody">This study examines Cevat Ey&amp;#252;p Ta&amp;#351;man, T&amp;#252;rkiye's pioneering petroleum geologist. Archival research reveals his multifaceted role: architect of systematic oil exploration, leader of the first major discovery, contributor to modern petroleum laws, and public educator.</span>
            </summary>
            <content type="html">
                &lt;b&gt;The founding actor of Türkiye's petroleum geology: Cevat Eyüp Taşman and his legacy in the national energy policies&lt;/b&gt;&lt;br&gt;
                Oğuz Mülayim&lt;br&gt;
                    Hist. Geo Space. Sci., 17, 25&#8211;35, https://doi.org/10.5194/hgss-17-25-2026, 2026&lt;br&gt;
                <p>This article examines the foundational role of Cevat Ey&amp;#252;p Ta&amp;#351;man (1893&amp;#8211;1956), T&amp;#252;rkiye's first petroleum geologist, by analyzing how his higher education in the United States and his professional experience with international oil companies established him as essential &amp;#8220;critical human capital&amp;#8221; for the Republic. Drawing on archival documents and primary sources, the study focuses on the period from his initial involvement in 1929 until his death in 1956. It structures his contributions around four foundational pillars that transformed the national oil enterprise: the technical-scientific pillar, established through systematic field research and global publications; the institutional pillar, realized by founding and leading national exploration bodies; the legal-regulatory pillar, marked by his pivotal role in drafting Petroleum Law No. 6326 (1954); and the intellectual-public pillar, demonstrated by his leadership in professional societies and public pedagogy. The research repositions Ta&amp;#351;man not only as a technical expert but also as a &amp;#8220;public intellectual&amp;#8221; who consistently aligned scientific knowledge with national development objectives. Accordingly, his legacy is assessed through these four pillars, which together underscore his enduring influence on T&amp;#252;rkiye's quest for energy independence.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-03-20T11:58:18+01:00</published>
            <updated>2026-03-20T11:58:18+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-17-13-2026</id>
            <title type="html">The first decade (1929&#8211;1939) of atmospheric electricity observations at &#346;wider Geophysical Observatory
            </title>
            <link href="https://doi.org/10.5194/hgss-17-13-2026"/>
            <summary type="html">
                &lt;b&gt;The first decade (1929–1939) of atmospheric electricity observations at Świder Geophysical Observatory&lt;/b&gt;&lt;br&gt;
                Anna Odzimek&lt;br&gt;
                    Hist. Geo Space. Sci., 17, 13&#8211;24, https://doi.org/10.5194/hgss-17-13-2026, 2026&lt;br&gt;
                In October 1929, measurements of the atmospheric potential gradient began to be routinely recorded at the Magnetic Observatory in &amp;#346;wider. There was a disruption and loss of the results of these measurements during World War II but the experience shaped the future of the observatory.
            </summary>
            <content type="html">
                &lt;b&gt;The first decade (1929–1939) of atmospheric electricity observations at Świder Geophysical Observatory&lt;/b&gt;&lt;br&gt;
                Anna Odzimek&lt;br&gt;
                    Hist. Geo Space. Sci., 17, 13&#8211;24, https://doi.org/10.5194/hgss-17-13-2026, 2026&lt;br&gt;
                <p>In October 1929, measurements of the atmospheric potential gradient (PG) began to be routinely recorded at the Magnetic Observatory in &amp;#346;wider, Poland. This started a new chapter in the history of the Observatory, in 1937 renamed the Geophysical Observatory in &amp;#346;wider. Two Benndorf electrometers recorded continuously until September 1939. War World II disrupted these observations as well as shattered efforts to publish the results of nearly a decade. Nevertheless, these early actions initiated by the Observatory management shaped its future as it became a contemporary atmospheric electricity station in the second half of the 20th century.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-02-06T11:58:18+01:00</published>
            <updated>2026-02-06T11:58:18+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-2026-3</id>
            <title type="html">Lofty aspirations born of sacrifice &#8211; In remembrance of Y. S. Ma, China's first female geologist, and her two colleagues who were murdered at the same time
            </title>
            <link href="https://doi.org/10.5194/hgss-2026-3"/>
            <summary type="html">
                &lt;b&gt;Lofty aspirations born of sacrifice – In remembrance of Y. S. Ma, China's first female geologist, and her two colleagues who were murdered at the same time&lt;/b&gt;&lt;br&gt;
                Jian Zhao Yin&lt;br&gt;
                    Hist. Geo Space. Sci. Discuss., doi:10.5194/hgss-2026-3,2026&lt;br&gt;
                    &lt;b&gt;Preprint withdrawn&lt;/b&gt; (discussion: closed, 11 comments)&lt;br&gt;
                As China's first scientific institution, Geological Survey of China created many firsts in Chinese geological education, research, and exploration. Unfortunately, following the murder of the geologist Chao by bandits in Yunnan in 1929, in 1944, three more geologists were killed in Guizhou, bordering Yunnan. Among the three were Ms. Ma, the only female geologist in China at the time, and Mr. Hsu and Chen. They were killed on the same day, at the ages of 25, 36, and 28 respectively.
            </summary>
            <content type="html">
                &lt;b&gt;Lofty aspirations born of sacrifice – In remembrance of Y. S. Ma, China's first female geologist, and her two colleagues who were murdered at the same time&lt;/b&gt;&lt;br&gt;
                Jian Zhao Yin&lt;br&gt;
                    Hist. Geo Space. Sci. Discuss., https://doi.org/10.5194/hgss-2026-3,2026&lt;br&gt;
                    &lt;b&gt;Preprint withdrawn&lt;/b&gt; (discussion: closed, 11 comments)&lt;br&gt;
                As China's first truly scientific education and research institution, the Geological Survey of China (GSC) achieved tremendous success within just a few years of its establishment, creating many firsts in Chinese geological education, research, and mineral exploration, and even some world firsts. However, this came at a heavy price; many geologists died young for various reasons. Especially during World War II, with the Japanese occupation of most of eastern and central China, almost all universities and research institutions in these developed regions had to relocate to the western rear areas of the war effort to continue geological surveys and research. At that time, bandits roamed freely in China, especially in the southwestern border regions, posing a significant threat and causing immense losses to the developing GSC. Following the tragic murder of the brilliant Chinese geologist Y. T. Chao by bandits in Zhaotong, Yunnan Province in 1929, 15 years later, in April 1944 during the War of Resistance against Japan, three more young geologists were killed by bandits in Guizhou Province, bordering eastern Yunnan. Among the three were Ms. Y.S. Ma, the only female geologist in China at the time, a young geologist fluent in five foreign languages &amp;#8203;&amp;#8203;despite never having been abroad, and Mr. T. Y. Hsu and Mr. K. Chen, both budding and accomplished geologists. They were killed on the same day, at the ages of 25, 36, and 28 respectively. This year marks the 82nd anniversary of their tragic deaths. This article is dedicated to these three young scholars who died before achieving their goals, leaving future generations deeply saddened.
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-02-03T11:58:18+01:00</published>
            <updated>2026-02-03T11:58:18+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-17-1-2026</id>
            <title type="html">Three historic tide gauge records from Svalbard
            </title>
            <link href="https://doi.org/10.5194/hgss-17-1-2026"/>
            <summary type="html">
                &lt;b&gt;Three historic tide gauge records from Svalbard&lt;/b&gt;&lt;br&gt;
                Philip L. Woodworth and Thorkild Aarup&lt;br&gt;
                    Hist. Geo Space. Sci., 17, 1&#8211;12, https://doi.org/10.5194/hgss-17-1-2026, 2026&lt;br&gt;
                Three historic tide gauge records from Svalbard were converted from 19<sup>th</sup&gt; century tabulations into computer files. They are good quality and can be used in modern tidal analysis. We confirmed previous findings on tidal constants and showed how little non-tidal variability in sea level there was at these times. One gauge used had an unusual design but it worked well and so deserves to be known. Biographical information is given on the people who acquired these data.
            </summary>
            <content type="html">
                &lt;b&gt;Three historic tide gauge records from Svalbard&lt;/b&gt;&lt;br&gt;
                Philip L. Woodworth and Thorkild Aarup&lt;br&gt;
                    Hist. Geo Space. Sci., 17, 1&#8211;12, https://doi.org/10.5194/hgss-17-1-2026, 2026&lt;br&gt;
                <p>Three historic tide gauge records from the Arctic archipelago of Svalbard have been converted from tabulations more than one century old into computer files. The records are found to be good quality and capable of being used in modern tidal analysis. The analyses confirm the findings on tidal constants by previous researchers and demonstrate how little non-tidal variability in sea level there was at these times. One of the tide gauges used was a crude contraption of a design not used before or since. Nevertheless, it appears to have worked well and so deserves to be better known.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-01-16T11:58:18+01:00</published>
            <updated>2026-01-16T11:58:18+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-16-65-2025</id>
            <title type="html">Geological investigations of the Lizard District, Cornwall, England: 1818&#8211;1883
            </title>
            <link href="https://doi.org/10.5194/hgss-16-65-2025"/>
            <summary type="html">
                &lt;b&gt;Geological investigations of the Lizard District, Cornwall, England: 1818–1883&lt;/b&gt;&lt;br&gt;
                Carl N. Drummond&lt;br&gt;
                    Hist. Geo Space. Sci., 16, 65&#8211;79, https://doi.org/10.5194/hgss-16-65-2025, 2025&lt;br&gt;
                The Lizard District of southern Cornwall is composed of a slab of ancient ocean crust containing rock types otherwise unknown in England. As such, the region has been of great interest to geologists for over two-hundred years. A review of scientific advances through the 19th century highlights the transition from generally field-based to detailed petrographic analyses.
            </summary>
            <content type="html">
                &lt;b&gt;Geological investigations of the Lizard District, Cornwall, England: 1818–1883&lt;/b&gt;&lt;br&gt;
                Carl N. Drummond&lt;br&gt;
                    Hist. Geo Space. Sci., 16, 65&#8211;79, https://doi.org/10.5194/hgss-16-65-2025, 2025&lt;br&gt;
                <p>A lower Paleozoic slab of oceanic lithosphere was obducted onto the southern margin of Avalonia during the Variscan orogeny and is now exposed throughout the Lizard District of Cornwall, England. This complexly faulted and metamorphosed region of mafic and ultramafic rocks has been the subject of geological investigation for over two hundred years. Herein the most significant scientific contributions made over a sixty-five-year interval from 1818 to 1883 are reviewed. Early workers, including Ashurst Majendie, Adam Sedgwick, John Rodgers, and Henry De la Beche, conducted field-based studies of the region, making lithologic observations and mapping contacts between the major rock units. Subsequently, an intense phase of investigation into the processes and products of contact and regional metamorphism in Cornwall and the Lake District informed and inspired the field and microscopical studies of the Lizard District by Thomas G. Bonney. Detailed consideration of the pioneering work of these 19th century geologists provides insights into their methodologies as well as an evolving understanding of the complex and enigmatic rocks of the Lizard.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2025-12-12T11:58:18+01:00</published>
            <updated>2025-12-12T11:58:18+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-16-51-2025</id>
            <title type="html">The role of point discharge in the historical development of atmospheric electricity
            </title>
            <link href="https://doi.org/10.5194/hgss-16-51-2025"/>
            <summary type="html">
                &lt;b&gt;The role of point discharge in the historical development of atmospheric electricity&lt;/b&gt;&lt;br&gt;
                Blair P. S. McGinness, R. Giles Harrison, Karen L. Aplin, and Martin W. Airey&lt;br&gt;
                    Hist. Geo Space. Sci., 16, 51&#8211;63, https://doi.org/10.5194/hgss-16-51-2025, 2025&lt;br&gt;
                Point discharge is an electrical process which occurs naturally in Earth's atmosphere. Like lightning, it has been observed both directly and indirectly for centuries. Several of the milestone investigations in atmospheric electricity have arisen through measuring point discharge. This work gives a history of various investigations involving the phenomenon and explains its central role in developments in atmospheric electricity.
            </summary>
            <content type="html">
                &lt;b&gt;The role of point discharge in the historical development of atmospheric electricity&lt;/b&gt;&lt;br&gt;
                Blair P. S. McGinness, R. Giles Harrison, Karen L. Aplin, and Martin W. Airey&lt;br&gt;
                    Hist. Geo Space. Sci., 16, 51&#8211;63, https://doi.org/10.5194/hgss-16-51-2025, 2025&lt;br&gt;
                <p>Point discharge, like lightning, is an atmospheric electricity process which has been observed directly and indirectly for centuries. Point discharge occurs when an electric field is enhanced at a point, causing local ionisation of the air and allowing a current to flow between the object and atmosphere. Point discharge sensors are simple instruments which measure the discharge currents caused by enhancements of the atmospheric electric field. In the early 20th Century, several milestone atmospheric electricity investigations were performed which employed the effects of naturally occurring point discharge currents and the measurements made by point discharge sensors. Point discharge was central to some of the arguments made in the proposal of the global atmospheric electric circuit, and the early evidence that was found to support this model. Point discharge sensors continued to be used throughout the 20th and 21st centuries, with understanding of their operations being developed further in this time.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2025-11-07T11:58:18+01:00</published>
            <updated>2025-11-07T11:58:18+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-16-41-2025</id>
            <title type="html">Historical background of Paleo Mega Lake of Rey
            </title>
            <link href="https://doi.org/10.5194/hgss-16-41-2025"/>
            <summary type="html">
                &lt;b&gt;Historical background of Paleo Mega Lake of Rey&lt;/b&gt;&lt;br&gt;
                Hadi Jarahi and Donya Namdar&lt;br&gt;
                    Hist. Geo Space. Sci., 16, 41&#8211;49, https://doi.org/10.5194/hgss-16-41-2025, 2025&lt;br&gt;
                This study reveals that a vast ancient lake once covered parts of central Iran, influencing regional culture and settlement. By analyzing old texts, maps, and environmental data, the research reconstructs the lake's size, timeline, and role in history. The findings suggest the lake lasted thousands of years before drying up due to climate shifts, offering new insights into how landscapes shaped early civilizations.
            </summary>
            <content type="html">
                &lt;b&gt;Historical background of Paleo Mega Lake of Rey&lt;/b&gt;&lt;br&gt;
                Hadi Jarahi and Donya Namdar&lt;br&gt;
                    Hist. Geo Space. Sci., 16, 41&#8211;49, https://doi.org/10.5194/hgss-16-41-2025, 2025&lt;br&gt;
                <p>Over the past decade, geological and historical evidence has increasingly suggested the existence of a vast ancient lake in central Iran, herein referred to as the Paleo Mega Lake of Rey (PAMELA). This study employs an interdisciplinary methodology to identify and geographically correlate historical references and terminologies associated with the lake. By analyzing over 350 sources, including travelogues, city histories, and ancient religious texts, we reconstructed the probable location, hydrological timeline, and cultural impact of the lake. Findings suggest that PAMELA has been referenced by various historical names such as Faraxkurt and Saveh Lake, and that it significantly influenced the livelihood of ancient communities. The integrated analysis points to a high probability of sustained water presence between 10&amp;#8201;000&amp;#8201;BCE and the 6th century&amp;#8201;CE.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2025-11-03T11:58:18+01:00</published>
            <updated>2025-11-03T11:58:18+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-16-31-2025</id>
            <title type="html">Paul J. Crutzen &#8211; interactions with friends and colleagues
            </title>
            <link href="https://doi.org/10.5194/hgss-16-31-2025"/>
            <summary type="html">
                &lt;b&gt;Paul J. Crutzen – interactions with friends and colleagues&lt;/b&gt;&lt;br&gt;
                Rolf Müller, Lennart Bengtsson, John Birks, John Burrows, Ruprecht Jaenicke, and Richard S. Stolarski&lt;br&gt;
                    Hist. Geo Space. Sci., 16, 31&#8211;40, https://doi.org/10.5194/hgss-16-31-2025, 2025&lt;br&gt;
                This paper reports a few anecdotes from the life of Paul J. Crutzen that were contributed by friends and colleagues. Taken together, these anecdotes should shed some light on the person that Paul was, as this is perhaps sometimes obscured when focusing solely on his many scientific achievements.
            </summary>
            <content type="html">
                &lt;b&gt;Paul J. Crutzen – interactions with friends and colleagues&lt;/b&gt;&lt;br&gt;
                Rolf Müller, Lennart Bengtsson, John Birks, John Burrows, Ruprecht Jaenicke, and Richard S. Stolarski&lt;br&gt;
                    Hist. Geo Space. Sci., 16, 31&#8211;40, https://doi.org/10.5194/hgss-16-31-2025, 2025&lt;br&gt;
                <p>Paul J. Crutzen was a brilliant scientist and a pioneer in atmospheric sciences. At the same time, he was a kind-hearted, humorous and pleasant person. Paul was deeply empathetic toward the personal lives of his  colleagues and students, always making time for those around him &amp;#8211; especially his family. This tribute brings together a series of anecdotes shared by friends and colleagues, offering a more intimate portrait of the man behind the science. Collectively, these reflections reveal aspects of Paul Crutzen that may be overlooked when focusing solely on his extraordinary scientific accomplishments; however, they were integral to his ability to achieve them.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2025-10-10T11:58:18+02:00</published>
            <updated>2025-10-10T11:58:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-16-23-2025</id>
            <title type="html">Revisiting the fall of the Veramin meteorite
            </title>
            <link href="https://doi.org/10.5194/hgss-16-23-2025"/>
            <summary type="html">
                &lt;b&gt;Revisiting the fall of the Veramin meteorite&lt;/b&gt;&lt;br&gt;
                Dan Holtstam and Ataollah Hassani&lt;br&gt;
                    Hist. Geo Space. Sci., 16, 23&#8211;29, https://doi.org/10.5194/hgss-16-23-2025, 2025&lt;br&gt;
                The meteorite "Veramin" fell in Persia ca. 1880. In the records, there are ambiguities about the event and the available sources were scrutinized in this review. The current official name, coined by meteoricist A. Brezina, is not supported by Iranian sources. A key document is a rediscovered label with the main mass of the meteorite. The indicated place of the event, probably occurring in February&amp;#8211;April 1880, is Booghin of in the historical Zarand district, 100 km NW from Veramin (Varamin).
            </summary>
            <content type="html">
                &lt;b&gt;Revisiting the fall of the Veramin meteorite&lt;/b&gt;&lt;br&gt;
                Dan Holtstam and Ataollah Hassani&lt;br&gt;
                    Hist. Geo Space. Sci., 16, 23&#8211;29, https://doi.org/10.5194/hgss-16-23-2025, 2025&lt;br&gt;
                <p>The Veramin meteorite, believed to have fallen in 1880, near Varamin, Tehran province, Iran (then Persia), is one of few witnessed falls of a mesosiderite, a rare type of stony-iron meteorite. In this review, it is described that historical records show inconsistencies regarding the fall, and consequently, the naming of the meteorite. The earliest printed account, by Ferdinand Dietzsch in 1881, reported that the meteorite fell near the village &amp;#8220;Karand&amp;#8221; east of Tehran, with a thunder-like sound. The Shah had ordered an examination of it. Later, meteoricist Aristides Brezina named it &amp;#8220;Veramin&amp;#8221;. Further historical accounts include descriptions by Iranian official Mohammad Hassan Khan Sani' od-Dowlah and the explorer Sven Hedin. A key document is a Persian text on a cardboard, preserved with the main meteorite mass in Tehran's Golestan Palace. Members of the nomadic Shahsevan-e Baghdadi tribal confederacy, who had winter settlements west of Tehran, are reported as eyewitnesses. The geologist Henry A. Ward provided a detailed description in 1901, confirming the meteorite's composition and securing a larger mass for analysis and distribution to museums. The exact location and date of the fall remain uncertain due to imprecise and conflicting sources. The most likely impact field is the Booghin-Eshtehard area west of Tehran, with the event happening sometime in the period February to April&amp;#160;1880. The original mentioning of &amp;#8220;Karand&amp;#8221; is a confusion with Zarand(ieh), 70&amp;#8201;km to the west of Varamin.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2025-09-18T11:58:18+02:00</published>
            <updated>2025-09-18T11:58:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-16-13-2025</id>
            <title type="html">Aurora records in the Spanish newspaper <i>Extremadura</i> for the period 1923&#8211;2017
            </title>
            <link href="https://doi.org/10.5194/hgss-16-13-2025"/>
            <summary type="html">
                &lt;b&gt;Aurora records in the Spanish newspaper Extremadura for the period 1923–2017&lt;/b&gt;&lt;br&gt;
                Constantino Sánchez Romero, Lucía Díaz-Condiño, Irene Tovar Hernández, Alejandro Jesús Pérez Aparicio, Víctor Manuel Sánchez Carrasco, María Cruz Gallego Herrezuelo, and José Manuel Vaquero&lt;br&gt;
                    Hist. Geo Space. Sci., 16, 13&#8211;22, https://doi.org/10.5194/hgss-16-13-2025, 2025&lt;br&gt;
                This article collects and analyzes reports of auroras published in the <em>Extremadura</em&gt; newspaper from 1923 to 2017. We identified 31 news items describing these events, including major auroras in 1926, 1938, 1957, and 1991. This research highlights the value of newspapers in reconstructing past solar activity.
            </summary>
            <content type="html">
                &lt;b&gt;Aurora records in the Spanish newspaper Extremadura for the period 1923–2017&lt;/b&gt;&lt;br&gt;
                Constantino Sánchez Romero, Lucía Díaz-Condiño, Irene Tovar Hernández, Alejandro Jesús Pérez Aparicio, Víctor Manuel Sánchez Carrasco, María Cruz Gallego Herrezuelo, and José Manuel Vaquero&lt;br&gt;
                    Hist. Geo Space. Sci., 16, 13&#8211;22, https://doi.org/10.5194/hgss-16-13-2025, 2025&lt;br&gt;
                <p>Aurora records are a valuable proxy for understanding historical solar behavior. This study explores historical records of auroras reported in the Spanish newspaper <i>Extremadura</i&gt; from 1923 to 2017. We found and analyzed 31 news articles, categorizing them into direct observations and general reports. The compiled news includes significant auroral events that occurred in 1926, 1938, 1950, 1956, 1957, 1958, and 1991. The news reports on aurorae visible not only in the Extremadura area but also across Spain and in other parts of the world. We have extracted information on the characteristics, places, timing, and societal impacts of auroras, in addition to providing information on these events included in previous scientific literature. This collection of auroral reports highlights historical newspapers as documentary sources for reconstructing solar activity and its effects on Earth.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2025-07-02T11:58:18+02:00</published>
            <updated>2025-07-02T11:58:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-16-1-2025</id>
            <title type="html">Contribution to the knowledge of early geotechnics during the 20th century: Laurits Bjerrum
            </title>
            <link href="https://doi.org/10.5194/hgss-16-1-2025"/>
            <summary type="html">
                &lt;b&gt;Contribution to the knowledge of early geotechnics during the 20th century: Laurits Bjerrum&lt;/b&gt;&lt;br&gt;
                Gonzalo Guillán-Llorente, Belén Muñoz-Medina, Antonio Lara-Galera, and Rubén Galindo-Aires&lt;br&gt;
                    Hist. Geo Space. Sci., 16, 1&#8211;12, https://doi.org/10.5194/hgss-16-1-2025, 2025&lt;br&gt;
                Karl Terzaghi reached out to Laurits Bjerrum in 1954, impressed by his paper on Norwegian quick clays' stability. At 36, Bjerrum, already a PhD and NGI director, emphasised practical research integration, influenced by centres like Imperial College London. He advocated for soil mechanics in civil engineering education and founded its chair in 1960. Bjerrum left a lasting legacy, earning international acclaim for his NGI work and collaborations with geotechnicians like Terzaghi and Casagrande.
            </summary>
            <content type="html">
                &lt;b&gt;Contribution to the knowledge of early geotechnics during the 20th century: Laurits Bjerrum&lt;/b&gt;&lt;br&gt;
                Gonzalo Guillán-Llorente, Belén Muñoz-Medina, Antonio Lara-Galera, and Rubén Galindo-Aires&lt;br&gt;
                    Hist. Geo Space. Sci., 16, 1&#8211;12, https://doi.org/10.5194/hgss-16-1-2025, 2025&lt;br&gt;
                <p>The founder of soil mechanics, Karl Terzaghi, took the initiative in 1954 to contact the Danish engineer Laurits Bjerrum, requesting to meet. Terzaghi wanted to meet the engineer who had written a paper on the stability of the unusual Norwegian quick clays at the European Slope Congress in Stockholm. Bjerrum was 36 years old at the time, had a PhD and was already director of the NGI (Norges Geotekniske Institutt &amp;#8211; Norwegian Geotechnical Institute). From his position as director of the NGI, he was actively involved in many varied consultancies, placing great value on the continuous interaction between practice and research. Bjerrum's strategy for establishing the NGI came from the experience of other research centres such as the BRS (Building Research Station) in Great Britain and Imperial College London. In addition, having lived through the Nazi occupation of Denmark, he was predisposed to be against the misuse of authority and established an open structure for the institute from its inception. Bjerrum was in close contact with the Norwegian Institution of Technology, and, in 1952, he succeeded in getting soil mechanics incorporated as a compulsory subject in the civil engineering degree. Subsequently, in 1960, the Chair of Soil Mechanics and Foundation Engineering was established. The first laboratory of this chair was equipped with material donated by the NGI. Bjerrum died young (54 years old), but he had built an excellent reputation through his work at the NGI and his contributions to international conferences, where he maintained a close relationship with the significant figures in geotechnics: Terzaghi, Skempton, Peck and Casagrande. He made regular trips to the USA, where he was a visiting professor at MIT (Massachusetts Institute of Technology) and received the highest international decorations.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2025-02-03T11:58:18+01:00</published>
            <updated>2025-02-03T11:58:18+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-15-81-2024</id>
            <title type="html">Historical evolution of the geomagnetic declination at the Royal Observatory of Madrid
            </title>
            <link href="https://doi.org/10.5194/hgss-15-81-2024"/>
            <summary type="html">
                &lt;b&gt;Historical evolution of the geomagnetic declination at the Royal Observatory of Madrid&lt;/b&gt;&lt;br&gt;
                Jose Manuel Tordesillas, Francisco Javier Pavón-Carrasco, Alberto Nuñez, and Ana Belén Anquela&lt;br&gt;
                    Hist. Geo Space. Sci., 15, 81&#8211;94, https://doi.org/10.5194/hgss-15-81-2024, 2024&lt;br&gt;
                In December 2021, the agonic line crossed the Royal Observatory of Madrid on its westward drift. The previous crossing by the agonic line, drifting eastward, is not accurately dated because declination measurements of that time are scarce. After collecting the data obtained in the Iberian Peninsula over the last 500 years and reducing them to ROM coordinates, a geomagnetic declination curve was generated. As a result, the previous cross ing been the agonic line was dated around the year 1652.
            </summary>
            <content type="html">
                &lt;b&gt;Historical evolution of the geomagnetic declination at the Royal Observatory of Madrid&lt;/b&gt;&lt;br&gt;
                Jose Manuel Tordesillas, Francisco Javier Pavón-Carrasco, Alberto Nuñez, and Ana Belén Anquela&lt;br&gt;
                    Hist. Geo Space. Sci., 15, 81&#8211;94, https://doi.org/10.5194/hgss-15-81-2024, 2024&lt;br&gt;
                <p>The agonic line, which represents geomagnetic declinations of 0&amp;#176;, recently crossed the Royal Observatory of Madrid (ROM) in December 2021, causing a shift in declination values from west to east. This event constitutes a notable milestone for this significant observatory, where the first geomagnetic observation series commenced around 1855 in Spain. In this work, taking advantage of the occurrence of this event, a detailed study has been conducted to investigate the historical evolution of the magnetic declination at the ROM to decipher prior occurrences of the agonic line crossing this place. Despite the ROM having hosted the first series of geomagnetic measurements in Spain, the present lack of geomagnetic measurements in this observatory makes it necessary to extend the declination measurements to other observatories distributed throughout the Iberian Peninsula to better define the passage of the agonic line since 1855 up to the present. For epochs prior to 1855, a bibliographic search for declination measurements conducted in the Iberian Peninsula has been carried out, complemented by historical data from the HISTMAG database. As a result, a time-continuous curve of geomagnetic declination is generated from 1590 to 2022 at the ROM coordinates. The declination curve reveals that the agonic line also crossed the ROM 400&amp;#160;years ago (around 1600), passing from western to eastern declination values.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2024-11-13T11:58:18+01:00</published>
            <updated>2024-11-13T11:58:18+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/hgss-15-71-2024</id>
            <title type="html">Lightning and thunder explanations in encyclopedias &#8211; from ancient Greece to Wikipedia
            </title>
            <link href="https://doi.org/10.5194/hgss-15-71-2024"/>
            <summary type="html">
                &lt;b&gt;Lightning and thunder explanations in encyclopedias – from ancient Greece to Wikipedia&lt;/b&gt;&lt;br&gt;
                Kristian Schlegel&lt;br&gt;
                    Hist. Geo Space. Sci., 15, 71&#8211;80, https://doi.org/10.5194/hgss-15-71-2024, 2024&lt;br&gt;
                The explanation of thunder and lightning in encyclopedias from ancient times to Wikipedia is described and discussed.
            </summary>
            <content type="html">
                &lt;b&gt;Lightning and thunder explanations in encyclopedias – from ancient Greece to Wikipedia&lt;/b&gt;&lt;br&gt;
                Kristian Schlegel&lt;br&gt;
                    Hist. Geo Space. Sci., 15, 71&#8211;80, https://doi.org/10.5194/hgss-15-71-2024, 2024&lt;br&gt;
                <p>After a brief introduction to encyclopedias, the explanation of lightning and thunder in well-known encyclopedias, from the works of Greek philosophers to encyclopedias of modern physics, is examined. Starting with Aristotle (who is not regarded as an encyclopedist but is very important for our topic), 10 out of more than 200 known encyclopedias are treated in some detail. This selection is certainly somewhat arbitrary, but it an attempt was made to choose encyclopedias which are highlights and which were widely circulated at their time. In antiquity and during the Middle Ages, the explanations of thunderstorms were generally quite different from the modern view, explaining, for instance, lightning as a consequence of thunder. Besides this, strange effects of lightning were often reported. Many authors of those times used the explanations of former encyclopedias, sometimes referring to earlier authors, often just plagiarizing. These ideas, unorthodox by our present understanding, persisted for almost 2 millennia in encyclopedias. From the middle of the 18th century onward, physical explanations began to emerge; these are still valid today. More and more correct details regarding lightning and thunder and the results of experiments have been reported in encyclopedias. It is also attempted in this paper to name the insights of other scientists which the authors of contemporary encyclopedias do not mention but which should have been available at the time. Finally, it is stated that, even today, several details regarding thunderstorms are not well understood.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2024-10-25T11:58:18+02:00</published>
            <updated>2024-10-25T11:58:18+02:00</updated>
        </entry>
</feed>