Sun Star

Results: 720



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111Observing Cycles, Seasons, and Storms Recent observational findings suggest that the 11(-ish) solar sunspot cycle is a pattern resulting from interaction, or interference, of large scale magnetic field bands that evolve

Observing Cycles, Seasons, and Storms Recent observational findings suggest that the 11(-ish) solar sunspot cycle is a pattern resulting from interaction, or interference, of large scale magnetic field bands that evolve

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Source URL: www.mssl.ucl.ac.uk

Language: English - Date: 2014-07-22 10:04:36
112Astronomy targets: April 2015 Unless stated otherwise, all times are for mid-month, for Birmingham UK and are GMT+1. Rise & set times are for 20 degrees above horizon. Dark & light times are nautical twilight times (Sun

Astronomy targets: April 2015 Unless stated otherwise, all times are for mid-month, for Birmingham UK and are GMT+1. Rise & set times are for 20 degrees above horizon. Dark & light times are nautical twilight times (Sun

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Source URL: www.broms-astro.co.uk

Language: English - Date: 2015-03-19 07:47:06
113Detection of Low-Level Activities in Solar-Analog Stars from the Emission Strengths of Ca II 3934 Line TAKEDA, Yoichi, TAJITSU, Akito, KAWANOMOTO, Satoshi, ANDO, Hiroyasu, SAKURAI, Takashi (NAOJ) HONDA, Satoshi

Detection of Low-Level Activities in Solar-Analog Stars from the Emission Strengths of Ca II 3934 Line TAKEDA, Yoichi, TAJITSU, Akito, KAWANOMOTO, Satoshi, ANDO, Hiroyasu, SAKURAI, Takashi (NAOJ) HONDA, Satoshi

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Source URL: www.nao.ac.jp

Language: English - Date: 2014-01-28 00:54:36
114Preface Our Sun is a fairly ordinary star, a bit brighter than most but not exceptionally so. There are many stars much bigger and brighter, while most stars are smaller and fainter. The Sun is not an especially variabl

Preface Our Sun is a fairly ordinary star, a bit brighter than most but not exceptionally so. There are many stars much bigger and brighter, while most stars are smaller and fainter. The Sun is not an especially variabl

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Source URL: www.cambridgeblog.org

Language: English - Date: 2014-04-25 09:43:59
115Evidence For Cloud-Cloud Collision and Parsec-Scale Stellar Feedback Within the L1641-N Region NAKAMURA, Fumitaka1, MIURA, Tomoya2, KITAMURA, Yoshimi3, SHIMAJIRI, Yoshito1 KAWABE, Ryohei1, AKASHI, Toshiya4, IKEDA, Norio3

Evidence For Cloud-Cloud Collision and Parsec-Scale Stellar Feedback Within the L1641-N Region NAKAMURA, Fumitaka1, MIURA, Tomoya2, KITAMURA, Yoshimi3, SHIMAJIRI, Yoshito1 KAWABE, Ryohei1, AKASHI, Toshiya4, IKEDA, Norio3

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Source URL: www.nao.ac.jp

Language: English - Date: 2013-02-04 00:48:05
116Direct Imaging of a Cold Jovian Planet Orbiting the Sun-like Star GJ 504 KUZUHARA, M.1, TAMURA, M.2/3, KUDO, T.4, JANSON, M.5/6, KANDORI, R.2, BRANDT, T. D.6/7 THALMANN, C.8, SPIEGEL, D.7, BILLER, B.9/10, CARSON, J.11, H

Direct Imaging of a Cold Jovian Planet Orbiting the Sun-like Star GJ 504 KUZUHARA, M.1, TAMURA, M.2/3, KUDO, T.4, JANSON, M.5/6, KANDORI, R.2, BRANDT, T. D.6/7 THALMANN, C.8, SPIEGEL, D.7, BILLER, B.9/10, CARSON, J.11, H

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Source URL: www.nao.ac.jp

Language: English - Date: 2015-03-23 03:19:20
117Chromospheres in Metal-Poor Stars Revealed from the He I 10830 Å Line (Tokai University) that two types of chromospheres exist: ——(1) The rotation-dependent chromospheric activity (seen in less-aged population I s

Chromospheres in Metal-Poor Stars Revealed from the He I 10830 Å Line (Tokai University) that two types of chromospheres exist: ——(1) The rotation-dependent chromospheric activity (seen in less-aged population I s

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Source URL: www.nao.ac.jp

Language: English - Date: 2012-07-25 04:23:18
118Detailed Density and Velocity Structures of the Protostellar Core B335 KURONO, Yasutaka, SAITO, Masao, KAMAZAKI, Takeshi, MORITA, Koh-Ichiro, KAWABE, Ryohei (NAOJ) In order to understand physical processes of lowmass sta

Detailed Density and Velocity Structures of the Protostellar Core B335 KURONO, Yasutaka, SAITO, Masao, KAMAZAKI, Takeshi, MORITA, Koh-Ichiro, KAWABE, Ryohei (NAOJ) In order to understand physical processes of lowmass sta

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Source URL: www.nao.ac.jp

Language: English - Date: 2014-01-28 00:54:38
119VIIRS Reflective Solar Band (RSB) Performance and Uncertainty Estimates Dr. Frank J. De Luccia The Aerospace Corporation - Reporting on behalf of entire VIIRS SDR Calibration/Validation team Suomi NPP SDR Product Review

VIIRS Reflective Solar Band (RSB) Performance and Uncertainty Estimates Dr. Frank J. De Luccia The Aerospace Corporation - Reporting on behalf of entire VIIRS SDR Calibration/Validation team Suomi NPP SDR Product Review

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Source URL: www.star.nesdis.noaa.gov

Language: English - Date: 2013-12-23 16:28:24
120Potential Members of Stellar Kinematic Groups within 30 pc of the Sun NAKAJIMA, Tadashi, MORINO, Jun-Ichi (NAOJ) Age dating of individual stars in general is a very difficult task. Usually groups of stars or stellar cl

Potential Members of Stellar Kinematic Groups within 30 pc of the Sun NAKAJIMA, Tadashi, MORINO, Jun-Ichi (NAOJ) Age dating of individual stars in general is a very difficult task. Usually groups of stars or stellar cl

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Source URL: www.nao.ac.jp

Language: English - Date: 2013-02-04 00:48:04