EBOOK - Advances in Geosciences - Solar Terrestial (Marc Duldig)

EBOOK - Những tiến bộ trong Khoa học địa chất - Năng lượng mặt trời - Tác giả: Marc Duldig (381 Trang).

By initial definition, the MM is a peculiar epoch in solar activity that took place at the time of Louis XIV, during which sunspots were almost absent.
After a systematic investigation of archive data by Ribes and Nesme-Ribes 9
The Solar Cycle at the Maunder Minimum Epoch 3
we know that, during the decade 1660–1670, the French astronomer Picard supported by the interest of Louis XIV observed the Sun as often as it was possible at that time and fixed the results in a way reasonably comparable with modern standards of scientific presentation. The result is that only one sunspot was observed during that period. The corresponding conclusion is
twofold. On one hand, the level of solar activity was extremely weak in comparison with periods after and just before the MM. On the other hand, the high reliability of the data implies that the only observed sunspot manifests some level of solar activity during the most deep phase of the MM. The point is that the sunspot formation is associated with a substantial toroidal magnetic field located somewhere deep inside the Sun. A maintenance of
such field needs some excitation mechanism which is usually identified with solar dynamo which in turn is usually cyclic.


The Solar Cycle at the Maunder Minimum Epoch 1
Hiroko Miyahara, Dmitry Sokoloff and Ilya G. Usoskin
Solar Coronal Plumes: Theoretical Concepts and Results 21
Manfred Cuntz Preflare Features in Microwaves and in Hard X-Rays 33
Ayumi Asai, Hiroshi Nakajima, Masumi Shimojo and Stephen M. White Nonextensive Entropy Approach to Space Plasma
Fluctuations and Turbulence 43
M. P. Leubner, Z. V¨or¨ os and W. Baumjohann
Simulation of Interplanetary Shock Wave Caused
by CME on August 25, 2001 65
Tomoya Ogawa, Mitsue Den, Takashi Tanaka and Kazuyuki Yamashita
Observation of the Influence of the January 15–17
Solar Storms to the Magnetic Field and Ionosphere of Indonesia 73
Clara Y. Yatini, Jiyo and Mamat Ruhimat
Observational Study of Solar Magnetic Active Phenomena by Huairou Vector Magnetograph 83
Hongqi Zhang
Development of Storm-Time Proton Total Energy Based on Multiobservation of NOAA Satellites
Keiko T. Asai, Tsutomu Nagatsuma, Tomoaki Hori and Yoshizumi Miyoshi On the Cross-Field Diffusion of Galactic Cosmic Rays into an ICME 115
K. Munakata, S. Yasue, C. Kato, J. Kota, M. Tokumaru,
M. Kojima, A. A. Darwish, T. Kuwabara and J. W. Bieber
On the Upper Limiting Energy of the Solar Diurnal
Anisotropy of Galactic Cosmic Ray Intensity 125
K. Munakata, S. Yasue, C. Kato, S. Akahane, M. Koyama,
S. Mori, A. A. Darwish, H. Tsuchiya, H. Onuma, K. Mizutani,
T. Yuda, M. Takita and J. Kota
Sector Boundary Crossings and Geomagnetic Activities 135
Shinichi Watari and Takashi Watanabe
Energetic Particle Composition Signatures in the
Earth Magnetotail 143
S. Y. Fu and Q.-G. Zong
The High Latitude Boundaries Under Extreme Solar Wind Conditions: A Cluster Perspective 163
H. Zhang, T. A. Fritz, Q.-G. Zong and P. W. Daly
The Magnetospheric Cusp: Structure and Dynamics 173
Q.-G. Zong, T. A. Fritz, H. Zhang, S. Y. Fu, X. Z. Zhou,
M. L. Goldstein, P. W. Daly, H. Reme, A. Balogh
and A. N. Fazakerley
Initial Results from the Simulation of the Halloween 2003 Storms 191
Ramon E. Lopez, Salvador Hernandez, Michael Wiltberger,
John Lyon and Charles Goodrich
Round-the-Clock Ground-Based Imaging Spectroscopy of Space Weather Effects on the Thermosphere and Ionosphere 201
Supriya Chakrabarti and D. Pallamraju Auroral Equatorward Boundary Observed by the
NOAA-17 Satellite 219
L. Xie, T. A. Fritz, Q.-G. Zong, Z. Y. Pu,
X. Z. Zhou and X. L. Li
Aurora-Associated Phenomena and the ePOP Mission 229
Ludmila M. Kagan
On the Importance of the Cross-Body Approach
in Planetary Aeronomy 239
Marina Galand, Anil Bhardwaj and Supriya Chakrabarti
Solar Terrestrial and Planetary Science Missions in
Asia–Oceania: Opportunities for Collaborative Research 249
Andrew W. Yau, Anil Bhardwaj, Iver H. Cairns, C. Z. Cheng,
Wing H. Ip, Yasumasa Kasaba, Kyoung W. Min,
Masato Nakamura and Yoshifumi Saito Incoherent Scatter Radarin Ionosphe.

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EBOOK - Những tiến bộ trong Khoa học địa chất - Năng lượng mặt trời - Tác giả: Marc Duldig (381 Trang).

By initial definition, the MM is a peculiar epoch in solar activity that took place at the time of Louis XIV, during which sunspots were almost absent.
After a systematic investigation of archive data by Ribes and Nesme-Ribes 9
The Solar Cycle at the Maunder Minimum Epoch 3
we know that, during the decade 1660–1670, the French astronomer Picard supported by the interest of Louis XIV observed the Sun as often as it was possible at that time and fixed the results in a way reasonably comparable with modern standards of scientific presentation. The result is that only one sunspot was observed during that period. The corresponding conclusion is
twofold. On one hand, the level of solar activity was extremely weak in comparison with periods after and just before the MM. On the other hand, the high reliability of the data implies that the only observed sunspot manifests some level of solar activity during the most deep phase of the MM. The point is that the sunspot formation is associated with a substantial toroidal magnetic field located somewhere deep inside the Sun. A maintenance of
such field needs some excitation mechanism which is usually identified with solar dynamo which in turn is usually cyclic.


The Solar Cycle at the Maunder Minimum Epoch 1
Hiroko Miyahara, Dmitry Sokoloff and Ilya G. Usoskin
Solar Coronal Plumes: Theoretical Concepts and Results 21
Manfred Cuntz Preflare Features in Microwaves and in Hard X-Rays 33
Ayumi Asai, Hiroshi Nakajima, Masumi Shimojo and Stephen M. White Nonextensive Entropy Approach to Space Plasma
Fluctuations and Turbulence 43
M. P. Leubner, Z. V¨or¨ os and W. Baumjohann
Simulation of Interplanetary Shock Wave Caused
by CME on August 25, 2001 65
Tomoya Ogawa, Mitsue Den, Takashi Tanaka and Kazuyuki Yamashita
Observation of the Influence of the January 15–17
Solar Storms to the Magnetic Field and Ionosphere of Indonesia 73
Clara Y. Yatini, Jiyo and Mamat Ruhimat
Observational Study of Solar Magnetic Active Phenomena by Huairou Vector Magnetograph 83
Hongqi Zhang
Development of Storm-Time Proton Total Energy Based on Multiobservation of NOAA Satellites
Keiko T. Asai, Tsutomu Nagatsuma, Tomoaki Hori and Yoshizumi Miyoshi On the Cross-Field Diffusion of Galactic Cosmic Rays into an ICME 115
K. Munakata, S. Yasue, C. Kato, J. Kota, M. Tokumaru,
M. Kojima, A. A. Darwish, T. Kuwabara and J. W. Bieber
On the Upper Limiting Energy of the Solar Diurnal
Anisotropy of Galactic Cosmic Ray Intensity 125
K. Munakata, S. Yasue, C. Kato, S. Akahane, M. Koyama,
S. Mori, A. A. Darwish, H. Tsuchiya, H. Onuma, K. Mizutani,
T. Yuda, M. Takita and J. Kota
Sector Boundary Crossings and Geomagnetic Activities 135
Shinichi Watari and Takashi Watanabe
Energetic Particle Composition Signatures in the
Earth Magnetotail 143
S. Y. Fu and Q.-G. Zong
The High Latitude Boundaries Under Extreme Solar Wind Conditions: A Cluster Perspective 163
H. Zhang, T. A. Fritz, Q.-G. Zong and P. W. Daly
The Magnetospheric Cusp: Structure and Dynamics 173
Q.-G. Zong, T. A. Fritz, H. Zhang, S. Y. Fu, X. Z. Zhou,
M. L. Goldstein, P. W. Daly, H. Reme, A. Balogh
and A. N. Fazakerley
Initial Results from the Simulation of the Halloween 2003 Storms 191
Ramon E. Lopez, Salvador Hernandez, Michael Wiltberger,
John Lyon and Charles Goodrich
Round-the-Clock Ground-Based Imaging Spectroscopy of Space Weather Effects on the Thermosphere and Ionosphere 201
Supriya Chakrabarti and D. Pallamraju Auroral Equatorward Boundary Observed by the
NOAA-17 Satellite 219
L. Xie, T. A. Fritz, Q.-G. Zong, Z. Y. Pu,
X. Z. Zhou and X. L. Li
Aurora-Associated Phenomena and the ePOP Mission 229
Ludmila M. Kagan
On the Importance of the Cross-Body Approach
in Planetary Aeronomy 239
Marina Galand, Anil Bhardwaj and Supriya Chakrabarti
Solar Terrestrial and Planetary Science Missions in
Asia–Oceania: Opportunities for Collaborative Research 249
Andrew W. Yau, Anil Bhardwaj, Iver H. Cairns, C. Z. Cheng,
Wing H. Ip, Yasumasa Kasaba, Kyoung W. Min,
Masato Nakamura and Yoshifumi Saito Incoherent Scatter Radarin Ionosphe.

LINK DOWNLOAD

Chuyên mục: C. Bài giảng C. Bài giảng chuyên ngành Nhiệt Lạnh (Heat and Refrigeration) C. Bài giảng kỹ thuật