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SCI收录的日全食高被引论文
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在Web of Science的SCI检索Total solar eclipse得知有270篇有关日全食论文（1975-2009），其中2009年有6篇题目中就有日全食的研究论文发表。详细论文摘要如下：
| 显示 1 条，共 6 条 |
| 作者: Davis, CJ (Davis, C. J.); Bell, SA (Bell, S. A.); Stamper, R (Stamper, R.); Poole, AWV (Poole, A. W. V.); McKinnell, LA (McKinnell, L. A.); Wilkinson, P (Wilkinson, P.) |
| 标题: A potential lag between the open solar magnetic source flux and solar EUV and X-ray emissions as measured by the Earth's ionosphere during total solar eclipses |
| 来源出版物: ANNALES GEOPHYSICAE, 27 (6): 2449-2456 2009 |
| 文献类型: Article |
| 作者关键词: Ionosphere; Solar radiation and cosmic ray effects; Solar physics, astrophysics, and astronomy; Corona and transition region; Magnetic fields |
| KeyWords Plus: FIELD |
| 摘要: Measurements of the ionospheric E-region during total solar eclipses have been used to provide information about the evolution of the solar magnetic field and EUV and X-ray emissions from the solar corona and chromosphere. By measuring levels of ionisation during an eclipse and comparing these measurements with an estimate of the unperturbed ionisation levels (such as those made during a control day, where available) it is possible to estimate the percentage of ionising radiation being emitted by the solar corona and chromosphere. Previously unpublished data from the two eclipses presented here are particularly valuable as they provide information that supplements the data published to date. The eclipse of 23 October 1976 over Australia provides information in a data gap that would otherwise have spanned the years 1966 to 1991. The eclipse of 4 December 2002 over Southern Africa is important as it extends the published sequence of measurements. Comparing measurements from eclipses between 1932 and 2002 with the solar magnetic source flux reveals that changes in the solar EUV and X-ray flux lag the open source flux measurements by approximately 1.5 years. We suggest that this unexpected result comes about from changes to the relative size of the limb corona between eclipses, with the lag representing the time taken to populate the coronal field with plasma hot enough to emit the EUV and X-rays ionising our atmosphere. |
| 地址: [Davis, C. J.; Stamper, R.] Rutherford Appleton Lab, Chilton OX11 0QX, Oxon, England; [Bell, S. A.] UK Hydrol Off, HM Naut Almanac Off, Taunton TA1 2DN, Somerset, England; [Poole, A. W. V.; McKinnell, L. A.] Rhodes Univ, Dept Phys & Elect, ZA-6140 Grahamstown, South Africa; [McKinnell, L. A.] Hermanus Magnet Observ, Hermanus, South Africa; [Wilkinson, P.] IPS Radio & Space Serv, Haymarket, NSW 1240, Australia |
| 通讯作者地址: Davis, CJ, Rutherford Appleton Lab, Chilton OX11 0QX, Oxon, England. |
| 电子邮箱地址: chris.davis@stfc.ac.uk |
| 被引频次: 0 |
| 来源文献页码计数: 8 |
| 显示 2 条，共 6 条 |
| 作者: Kilcik, A (Kilcik, A.); Sigismondi, C (Sigismondi, C.); Rozelot, JP (Rozelot, J. P.); Guhl, K (Guhl, K.) |
| 标题: Solar Radius Determination from Total Solar Eclipse Observations on 29 March 2006 |
| 来源出版物: SOLAR PHYSICS, 257 (2): 237-250 JUL 2009 |
| 文献类型: Article |
| 作者关键词: Sun: activity; Sun: diameter; Sun: eclipses |
| KeyWords Plus: 11-YEAR ACTIVITY CYCLE; LUNAR OCCULTATIONS; DISK SEXTANT; DIAMETER; SUN; STRATIFICATION; OBLATENESS; CONSTANCY |
| 摘要: Solar diameter measurements have been made nearly continuously through different techniques for more than three centuries. They were obtained mainly with ground-based instruments except for some recent estimates deduced from space observations. One of the main problems in such space data analysis is that, up to now, it has been difficult to obtain an absolute value owing to the absence of an internally calibrated system. Eclipse observations provide a unique opportunity to give an absolute angular scale to the measurements, leading to an absolute value of the solar diameter. However, the problem is complicated by the Moon limb, which presents asphericity because of the mountains. We present a determination of the solar diameter derived from the total solar eclipse observation in Turkey and Egypt on 29 March 2006. We found that the solar radius carried back to 1 AU was 959.22 +/- 0.04 arcsec at the time of the observations. The inspection of the compiled 19 modern eclipses data, with solar activity, shows that the radius changes are nonhomologous, an effect that may explain the discrepancies found in ground-based measurements and implies the role of the shallow subsurface layers (leptocline) of the Sun. |
| 地址: [Kilcik, A.] Akdeniz Univ, Dept Phys, Fac Art & Sci, TR-07058 Antalya, Turkey; [Sigismondi, C.] Univ Roma La Sapienza, ICRA Int Ctr Relativist Astrophys, I-00185 Rome, Italy; [Sigismondi, C.] Univ Nice Sophia Antipolis, Fizeau Dept, F-06108 Nice, France; [Rozelot, J. P.] Univ Nice Sophia Antipolis, Fizeau Dept, CNRS, OCA,UMR 6225, F-06130 Grasse, France; [Guhl, K.] Archenhold Sternwarte, Berlin, Germany; [Guhl, K.] IOTA ES Int Occultat Timing Assoc, European Sect, D-12435 Berlin, Germany |
| 通讯作者地址: Kilcik, A, Akdeniz Univ, Dept Phys, Fac Art & Sci, TR-07058 Antalya, Turkey. |
| 电子邮箱地址: alikilcik@akdeniz.edu.tr; sigismondi@icra.it; Jean-Pierre.Rozelot@obs-azur.fr; kguhl@astw.de |
| 被引频次: 0 |
| DOI: 10.1007/s11207-009-9378-x |
| 来源文献页码计数: 14 |
| 显示 3 条，共 6 条 | ||||||
| 作者: Pasachoff, JM (Pasachoff, Jay M.) | ||||||
| 标题: Scientific observations at total solar eclipses | ||||||
| 来源出版物: RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 9 (6): 613-634 JUN 2009 | ||||||
| 文献类型: Review | ||||||
| 作者关键词: Sun: eclipses | ||||||
| KeyWords Plus: 26 FEBRUARY 1998; PERIOD CORONAL OSCILLATIONS; HIGH-FREQUENCY OSCILLATIONS; WHITE-LIGHT CORONA; SHADOW BANDS; ELECTRON-TEMPERATURE; ALFVEN WAVES; SPECTRUM; LOOPS; LINE | ||||||
| 摘要: The occasion of the longest totality of an eclipse in the 18 yr 11(1)/(3) d saros cycle leads to taking stock of the scientific value of ground-based eclipse observations in this space age. Though a number of space satellites from the U.S., Europe, Japan, and Russia study the Sun, scientists at eclipses can observe the solar chromosphere and corona at higher spatial resolution, at higher temporal resolution, and at higher spectral resolution than are possible aloft. Furthermore, eclipse expeditions can transport a wide variety of state-of-the-art equipment to the path of totality. Thus, for at least some years to come, solar eclipse observations will remain both scientifically valuable and cost-effective ways to study the outer solar atmosphere. | ||||||
| 地址: [Pasachoff, Jay M.] Williams Coll, Hopkins Observ, Williamstown, MA 01267 USA; [Pasachoff, Jay M.] CALTECH, Pasadena, CA 91125 USA | ||||||
| 通讯作者地址: Pasachoff, JM, Williams Coll, Hopkins Observ, Williamstown, MA 01267 USA. | ||||||
| 电子邮箱地址: eclipse@williams.edu | ||||||
| 基金资助致谢: | ||||||
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My expeditions have been partly supported by grants, most recently ATM-0552116, from the Solar Terrestrial Research Program of the U.S. National Science Foundation's Division of Atmospheric Sciences, the Committee for Research and Exploration of the National Geographic Society, NASA's Planetary Astronomy Division for the CCD cameras, Sigma Xi, and the Rob Spring Fund and the Ryan Patrick Gaishin Fund at Williams College. I thank Bryce A. Babcock, Steven P. Souza of Williams College, Robert Lucas of the University of Sydney, Alphya Nesterenkc, of the State University of Novosibirsk and Igor Nesterenko of the Budker Institute of Nuclear Physics, and John H. Seiradakis of the Aristotle University of Thessaloniki, Greece, for their assistance and colleagueship. We are pleased with the continued collaboration of Jonathan Kern of the Carnegie Observatories and of Wendy Carlos. J.M.P. thanks Michael Brown and the Division of Geological and Planetary Sciences at Caltech for their hospitality. Pasachoff and his team also appreciate the collaboration of Yihua Yan of the National Astronomical Observatories of China, Jin Zhu of the Beijing Planetarium, and Lin Lan of Hangzhou High School, during the two years of eclipse-planning for the 2009 totality. He thanks Serge Koutchmy and Luc Dame in France and Jagdev Singh in India for their comments on his manuscript. |
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| 被引频次: 0 | ||||||
| 来源文献页码计数: 22 |
| 显示 4 条，共 6 条 | ||||||||
| 作者: Qu, ZQ (Qu, Z. Q.); Zhang, XY (Zhang, X. Y.); Xue, ZK (Xue, Z. K.); Dun, GT (Dun, G. T.); Zhong, SH (Zhong, S. H.); Liang, HF (Liang, H. F.); Yan, XL (Yan, X. L.); Xu, CL (Xu, C. L.) | ||||||||
| 标题: LINEAR POLARIZATION OF FLASH SPECTRUM OBSERVED FROM A TOTAL SOLAR ECLIPSE IN 2008 | ||||||||
| 来源出版物: ASTROPHYSICAL JOURNAL LETTERS, 695 (2): L194-L197 APR 20 2009 | ||||||||
| 文献类型: Article | ||||||||
| 作者关键词: polarization; Sun: chromosphere; Sun: corona | ||||||||
| KeyWords Plus: MAGNETIC-FIELDS; WINDOW | ||||||||
| 摘要: We measured linear polarization signals of the flash spectrum ranging from 502.5 nm to 528.5 nm after second contact of a total solar eclipse which occurred on 2008 August 1 in China. A large group of spectral lines (especially those lines produced by neutral iron, neutral copper, and as carbon molecules) are found with very high polarization degrees relative to the continuum polarization, and the linear polarization spectrum is more abundantly structured than the flash spectrum itself. According to the observational result, we conclude that coherent scattering and scattering geometry as well as other mechanisms may together play a very important role in producing the high polarization amplitudes. This will help us deepen our understanding of the physical conditions of the solar upper atmospheres and the physical processes occurring there. | ||||||||
| 地址: [Qu, Z. Q.; Zhang, X. Y.; Xue, Z. K.; Dun, G. T.; Zhong, S. H.; Yan, X. L.] Chinese Acad Sci, Natl Astron Observ, Yunnan Astron Observ, Kunming 650011, Yunnan, Peoples R China; [Liang, H. F.; Xu, C. L.] Yunnan Normal Univ, Kunming 650135, Yunnan, Peoples R China | ||||||||
| 通讯作者地址: Qu, ZQ, Chinese Acad Sci, Natl Astron Observ, Yunnan Astron Observ, Kunming 650011, Yunnan, Peoples R China. | ||||||||
| 基金资助致谢: | ||||||||
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The authors are indebted to J.O. Stenflo and C. U. Keller for their very constructive suggestions. This work is supported by the National Astronomical Observatories, Chinese Academy of Sciences, the National Science Foundation of China (NSFC) under grants 10673031 and 40636031, and National Basic Research Program of China 973 under grant G2006CB806301. |
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| 被引频次: 1 | ||||||||
| DOI: 10.1088/0004-637X/695/2/L194 | ||||||||
| 来源文献页码计数: 4 |
| 显示 5 条，共 6 条 |
| 作者: Pleijel, H (Pleijel, Hakan) |
| 标题: Observations of temperature and air humidity during the total solar eclipse 29 March 2006 at Side, Turkey |
| 来源出版物: METEOROLOGISCHE ZEITSCHRIFT, 18 (1): 107-109 2009 |
| 文献类型: Article |
| KeyWords Plus: 11 AUGUST 1999 |
| 摘要: Air temperature and relative humidity were measured during the total solar eclipse 29 March 2006 at Side, Turkey (N36 degrees 45.95'; E31 degrees 23.71') at screen height. The temperature was reduced by 5.0 degrees C from the start of the eclipse until totality and increased by 4.3 degrees C after totality. An overestimation of the temperature drop during the eclipse due to a radiation effect oil the temperature measurement of similar to 0.5 degrees C cannot be excluded. The relative humidity followed an inverse pattern compared to air temperature during the eclipse. In contrast, the vapour pressure varied little during the eclipse and did not appear to be systematically affected by the eclipse conditions. |
| 地址: Univ Gothenburg, S-40530 Gothenburg, Sweden |
| 通讯作者地址: Pleijel, H, Univ Gothenburg, POB 461, S-40530 Gothenburg, Sweden. |
| 电子邮箱地址: hakan.pleijel@dpes.gu.se |
| 被引频次: 0 |
| DOI: 10.1127/0941-2948/2008/0324 |
| 来源文献页码计数: 3 |
| 显示 6 条，共 6 条 |
| 作者: Lala, S (Lala, Sukumar); Sharma, S (Sharma, Seema); Chakrabarti, S (Chakrabarti, Swati); Chakravarty, N (Chakravarty, Nabajit) |
| 标题: ATMOSPHERIC PRESSURE PERTURBATION DURING TOTAL SOLAR ECLIPSE |
| 来源出版物: MAUSAM, 60 (1): 103-106 JAN 2009 |
| 文献类型: Letter |
| 地址: [Lala, Sukumar] Meteorol Off, Ganjam, Orissa, India; [Sharma, Seema] Reg Met Ctr, Bombay, Maharashtra, India; [Chakrabarti, Swati] Met Observ, Cooch Behar, W Bengal, India; [Chakravarty, Nabajit] Indian Assoc Cultivat Sci, Calcutta, India |
| 通讯作者地址: Lala, S, Meteorol Off, Ganjam, Orissa, India. |
| 电子邮箱地址: sukumarlala@gmail.com; nabajit_c@yahoo.com |
| 被引频次: 0 |
| 来源文献页码计数: 4 |
有关日全食的高被引论文如下：
| 1. | 标题: CORONAL DENSITY AND TEMPERATURE STRUCTURE FROM COORDINATED OBSERVATIONS ASSOCIATED WITH THE TOTAL SOLAR ECLIPSE OF 1988 MARCH 18 作者: GUHATHAKURTA M, ROTTMAN GJ, FISHER RR, et al. 来源出版物: ASTROPHYSICAL JOURNAL 卷: 388 期: 2 页: 633-643 子辑: Part 1 出版年: APR 1 1992 被引频次: 34 |
| 2. | 标题: SUBMILLIMETER OBSERVATIONS OF THE 1991 JULY 11 TOTAL SOLAR ECLIPSE 作者: EWELL MW, ZIRIN H, JENSEN JB, et al. 来源出版物: ASTROPHYSICAL JOURNAL 卷: 403 期: 1 页: 426-433 子辑: Part 1 出版年: JAN 20 1993 被引频次: 32 |
| 3. | 标题: CONVULSIVE THRESHOLD IN HUMANS AND RATS AND MAGNETIC-FIELD CHANGES - OBSERVATIONS DURING TOTAL SOLAR ECLIPSE 作者: KESHAVAN MS, GANGADHAR BN, GAUTAM RU, et al. 来源出版物: NEUROSCIENCE LETTERS 卷: 22 期: 2 页: 205-208 出版年: 1981 被引频次: 25 |
| 4. | 标题: Detection of short-period coronal oscillations during the total solar eclipse of 24 October, 1995 作者: Singh J, Cowsik R, Raveendran AV, et al. 来源出版物: SOLAR PHYSICS 卷: 170 期: 2 页: 235-252 出版年: FEB 1997 被引频次: 24 |
| 5. | 标题: FLUCTUATIONS IN COLUMN OZONE DURING THE TOTAL SOLAR ECLIPSE OF JULY 11, 1991 作者: MIMS FM, MIMS ER 来源出版物: GEOPHYSICAL RESEARCH LETTERS 卷: 20 期: 5 页: 367-370 出版年: MAR 5 1993 被引频次: 20 |
| 6. | 标题: OBSERVATIONS OF A SONIC-SCATTERING LAYER DURING TOTAL SOLAR ECLIPSE, 30 JUNE, 1973 作者: KAMPA EM 来源出版物: DEEP-SEA RESEARCH 卷: 22 期: 6 页: 417-& 出版年: 1975 被引频次: 19 |
| 7. | 标题: PHOTOMETRIC STUDY OF CHROMOSPHERIC AND CORONAL SPIKES OBSERVED DURING TOTAL SOLAR ECLIPSE OF 30 JUNE, 1973 作者: KOUTCHMY S, STELLMACHER G 来源出版物: SOLAR PHYSICS 卷: 49 期: 2 页: 253-265 出版年: 1976 被引频次: 18 |
| 8. | 标题: CORONAL EMISSION-LINE PROFILE OBSERVATIONS AT TOTAL SOLAR ECLIPSES .2. 30 MAY 1965 RESULTS, DECONVOLUTION AND INTERPRETATION 作者: LIEBENBERG DH, BESSEY RJ, WATSON B 来源出版物: SOLAR PHYSICS 卷: 44 期: 2 页: 345-359 出版年: 1975 被引频次: 18 |
| 9. | 标题: Short-period intensity oscillations in the solar corona observed during the total solar eclipse of 26 February 1998 作者: Cowsik R, Singh J, Saxena AK, et al. 来源出版物: SOLAR PHYSICS 卷: 188 期: 1 页: 89-98 出版年: AUG 1999 被引频次: 15 |
| 10. | 标题: POLARIZATION OF THE GREEN LINE OBSERVED AT THE 1973 JUNE 30 TOTAL SOLAR ECLIPSE 作者: PICAT JP, FELENBOK P 来源出版物: ASTRONOMY AND ASTROPHYSICS 卷: 75 期: 1-2 页: 176-181 出版年: 1979 被引频次: 15 |
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