The role of activity complexes in the distribution of solar magnetic fields.

Bibcode
1990PDHO....7...80G
García de La Rosa, J. I.; Reyes, R. C.
Bibliographical reference

Publications of Debrecen Heliophysical Observatory, Vol. 7, p. 80 - 83

Advertised on:
0
1990
Number of authors
2
IAC number of authors
0
Citations
0
Refereed citations
0
Description
Using published data on the large-scale distribution of solar activity, the authors conclude that the longlived coronal holes are formed and maintained by the unbalanced magnetic flux which developes at both extremes of the complexes of activity.
Type
Non-refereed
Solar coronal holes
Solar magnetic fields
Solar activity

It may interest you

  • Non-refereed
    The TESS TTV Follow-up Program: Revealing Volatile-Rich Terrestrial Planets Around M Stars
    Models predict that water-rich planets may be common around low-mass stars, but definitive evidence for the existence of water worlds has remained elusive. Recent JWST observations of sub-Neptune sized planets orbiting nearby M dwarfs found atmospheres enriched in CH4, CO2 and H2O, but the enrichment mechanism is debated. To answer this question
    Greklek-McKeon, Michael et al.

    Advertised on:

    7
    2024
    Bibcode
    2024tsc3.confE..21G
    Citations
    0
  • Non-refereed
    The instrumentation plan of the 10.4m GTC telescope
    The 10.4m Gran Telescopio Canarias (GTC) was designed to be a versatile telescope, able to serve a wide scientific community. To this aim, various focal stations have been equipped, including a Cassegrain, two Nasmyth foci, and four folded-Cassegrain stations. This allows an ambitious instrumentation plan to be developed. We present the latest
    Corradi, Romano L. M. et al.

    Advertised on:

    7
    2024
    Bibcode
    2024SPIE13096E..0HC
    Citations
    0
  • Non-refereed
    Design and fabrication of fold mirror (M3) system for New Robotic Telescope
    The New Robotic Telescope (NRT) is an autonomous telescope that can operate multiple instruments at the Cassegrain focal station and the straight-through port. The optical beam is directed to the ports by a fold mirror subsystem in the focal station assembly. The fold mirror is elliptical in shape, manufactured by Instituto Nazionale di Astrofisica
    Ranjbar, Ali et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13094E..2HR
    Citations
    0