Stellar magnetic field

Results: 48



#Item
1

FOR RELEASE: 9:00 AM EST, January 7, 2004 PLANET CREATES A STELLAR STORM FIRST EVIDENCE OF AN EXTRA-SOLAR PLANET WITH A MAGNETIC FIELD

Add to Reading List

Source URL: www.uta.edu

Language: English - Date: 2015-06-10 15:36:24
    2Proc. July 2007 Conf. on Unsolved Problems in Stellar Physics, Amer. Inst. of Physics, in press.  Confinement of the Sun’s interior magnetic field: some exact boundary-layer solutions T. S. Wood and M. E. McIntyre Depa

    Proc. July 2007 Conf. on Unsolved Problems in Stellar Physics, Amer. Inst. of Physics, in press. Confinement of the Sun’s interior magnetic field: some exact boundary-layer solutions T. S. Wood and M. E. McIntyre Depa

    Add to Reading List

    Source URL: www.atm.damtp.cam.ac.uk

    Language: English - Date: 2013-10-19 17:24:24
      3Theories of the solar cycle : a critical view  arXiv:1004.4545v1 [astro-ph.SR] 26 Apr 2010 H.C. Spruit∗ Max Planck Institute for Astrophysics

      Theories of the solar cycle : a critical view arXiv:1004.4545v1 [astro-ph.SR] 26 Apr 2010 H.C. Spruit∗ Max Planck Institute for Astrophysics

      Add to Reading List

      Source URL: spd.aas.org

      Language: English - Date: 2010-05-11 15:03:16
      4Copyright by Michael Houston Montgomery 1993  The Frequency Splitting of Multiplets in the Oscillations

      Copyright by Michael Houston Montgomery 1993 The Frequency Splitting of Multiplets in the Oscillations

      Add to Reading List

      Source URL: www.as.utexas.edu

      Language: English - Date: 2003-09-26 16:38:01
      5Univ.-Prof. Dr. Bodo Ziegler Leiter des Instituts Einladung zum Seminar über

      Univ.-Prof. Dr. Bodo Ziegler Leiter des Instituts Einladung zum Seminar über

      Add to Reading List

      Source URL: typo3.univie.ac.at

      Language: English - Date: 2015-05-11 09:09:28
      6Question 4. Starting from radiative transfer equation, suppose the source function is a linear a b ,v function of vertical optical depth S ,v (a) Please explain what is limb darkening effect using the surface intensiti

      Question 4. Starting from radiative transfer equation, suppose the source function is a linear a b ,v function of vertical optical depth S ,v (a) Please explain what is limb darkening effect using the surface intensiti

      Add to Reading List

      Source URL: www.astro.ncu.edu.tw

      Language: English - Date: 2014-05-12 00:06:46
      7Light sources / Space plasmas / Plasma physics / Stellar astronomy / Planetary science / Aurora / Magnetic field / Sun / Star / Physics / Electromagnetism / Astronomy

      Homework questions for Ch. 4 Vol. IV Q1: Let’s define r0 as the point along a magnetic field line of the Astrospheric Magnetic Field (AMF) at which the field line is open to space by the stellar wind (this is the point

      Add to Reading List

      Source URL: www.heliophysics.ucar.edu

      Language: English - Date: 2014-07-14 17:17:11
      8Observing 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

      Add to Reading List

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

      Language: English - Date: 2014-07-22 10:04:36
      9Mon. Not. R. Astron. Soc. 000, 1–Printed 15 JanuaryMN LATEX style file v2.2)

      Mon. Not. R. Astron. Soc. 000, 1–Printed 15 JanuaryMN LATEX style file v2.2)

      Add to Reading List

      Source URL: users.monash.edu.au

      Language: English - Date: 2008-01-15 18:05:23
      10The Inner Structure of Collisionless Magnetic Reconnection ZENITANI, Seiji (NAOJ) Magnetic reconnection is a driving engine of solar flares, stellar flares, and quite probably bursty events

      The Inner Structure of Collisionless Magnetic Reconnection ZENITANI, Seiji (NAOJ) Magnetic reconnection is a driving engine of solar flares, stellar flares, and quite probably bursty events

      Add to Reading List

      Source URL: www.nao.ac.jp

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