Solar cycle 24

Results: 80



#Item
21ROM SAF CDOP-2 Visiting Scientist Report 24: Testing a new model for the residual ionospheric correction error in GPS radio occultation retrievals Julia Danzer

ROM SAF CDOP-2 Visiting Scientist Report 24: Testing a new model for the residual ionospheric correction error in GPS radio occultation retrievals Julia Danzer

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Source URL: www.romsaf.org

Language: English - Date: 2014-09-26 07:12:12
22Solar Cycle 24, W. Dean Pesnell, prepared May 24, PREDICTIONS OF SOLAR CYCLE 24 William Dean Pesnell

Solar Cycle 24, W. Dean Pesnell, prepared May 24, PREDICTIONS OF SOLAR CYCLE 24 William Dean Pesnell

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Source URL: legacy-www.swpc.noaa.gov

Language: English - Date: 2012-01-31 09:07:21
23Unusual Migration of the Prominence Activities in the Southern Hemisphere during Cycle 23‒24 SHIMOJO, Masumi (NAOJ) The solar activity in Cycle 23‒24 shows differences

Unusual Migration of the Prominence Activities in the Southern Hemisphere during Cycle 23‒24 SHIMOJO, Masumi (NAOJ) The solar activity in Cycle 23‒24 shows differences

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Source URL: www.nao.ac.jp

Language: English - Date: 2015-03-23 03:19:20
24GEOPHYSICAL RESEARCH LETTERS, VOL. 38, L20108, doi:2011GL049227, 2011 The prelude to the deep minimum between solar cycles 23 and 24: Interplanetary scintillation signatures in the inner heliosphere P. Janardhan

GEOPHYSICAL RESEARCH LETTERS, VOL. 38, L20108, doi:2011GL049227, 2011 The prelude to the deep minimum between solar cycles 23 and 24: Interplanetary scintillation signatures in the inner heliosphere P. Janardhan

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Source URL: www.prl.res.in

Language: English - Date: 2013-05-06 15:44:28
25Solar cycle 24 looks set to be the weakest of the space age, both in terms of sunspot number and the heliospheric magnetic field (HMF). The most recent observations of the solar polar field polarities suggest the Sun is

Solar cycle 24 looks set to be the weakest of the space age, both in terms of sunspot number and the heliospheric magnetic field (HMF). The most recent observations of the solar polar field polarities suggest the Sun is

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

- Date: 2013-04-04 05:48:03
    26The Astrophysical Journal, 700:L154–L157, 2009 August 1  Cdoi:637XL154

    The Astrophysical Journal, 700:L154–L157, 2009 August 1  Cdoi:637XL154

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    Source URL: climate.arm.ac.uk

    Language: English - Date: 2009-07-31 04:36:46
    27The difference between CMEs and solar flares

    The difference between CMEs and solar flares

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    Source URL: phys.org

    Language: English - Date: 2015-05-04 08:42:17
    28เปิดสายด่วน 1111 กด 5 ให้ข้อมูลน้ำท่วมตลอด 24 ชม

    เปิดสายด่วน 1111 กด 5 ให้ข้อมูลน้ำท่วมตลอด 24 ชม

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    Source URL: www.tei.or.th

    Language: English - Date: 2011-10-12 00:11:56
    29Recent in situ solar wind observations indicate that solar wind charge-state (O7/C6 ratio) and alpha composition is evolving through the extended deep solar minimum between solar cycle 23 and 24. For solar wind of a give

    Recent in situ solar wind observations indicate that solar wind charge-state (O7/C6 ratio) and alpha composition is evolving through the extended deep solar minimum between solar cycle 23 and 24. For solar wind of a give

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    Source URL: solarorbiter4.org

    Language: English - Date: 2011-05-17 20:49:44
    30The longitudinal spread of solar energetic particles – a case study: The January 17, 2010 SEP event N. Dresing, R. Gómez-Herrero, A. Klassen, B. Heber, Y. Kartavykh, W. Dröge During the rising phase of solar cycle 24

    The longitudinal spread of solar energetic particles – a case study: The January 17, 2010 SEP event N. Dresing, R. Gómez-Herrero, A. Klassen, B. Heber, Y. Kartavykh, W. Dröge During the rising phase of solar cycle 24

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    Source URL: solarorbiter4.org

    Language: English - Date: 2011-05-17 20:48:43