The prelude to the deep minimum between solar cycles 23 and 24: Interplanetary scintillation signatures in the inner heliosphere
Abstract
Extensive interplanetary scintillation (IPS) observations at 327 MHz obtained between 1983 and 2009 clearly show a steady and significant drop in the turbulence levels in the entire inner heliosphere starting from around ∼1995. We believe that this large-scale IPS signature, in the inner heliosphere, coupled with the fact that solar polar fields have also been declining since ∼1995, provide a consistent result showing that the buildup to the deepest minimum in 100 years actually began more than a decade earlier.
- Publication:
-
Geophysical Research Letters
- Pub Date:
- October 2011
- DOI:
- arXiv:
- arXiv:1110.0437
- Bibcode:
- 2011GeoRL..3820108J
- Keywords:
-
- Interplanetary Physics: Coronal mass ejections (4305;
- 7513);
- Interplanetary Physics: Interplanetary magnetic fields;
- Interplanetary Physics: Plasma waves and turbulence;
- Interplanetary Physics: Solar cycle variations (7536);
- Interplanetary Physics: Solar wind plasma;
- Astrophysics - Solar and Stellar Astrophysics;
- Physics - Space Physics
- E-Print:
- 9 pages, 4 figures, accepted for publication in Geophysical Research Letters on 28 September 2011