Arşiv Cuma, 20 Haziran 2003 görüntüleniyor
Güneş aktivite raporu
Bu raporda bahsedilen herhangi bir güneş lekesi, Uzay Hava Tahmin Merkezi (SWPC) tarafından uygulanan bir ölçekleme faktörüne sahiptir. SWPC ölçekleme faktörü nedeniyle güneş lekeleri, bilimsel kalitedeki verilere göre %42 daha küçük olarak rapor edilmektedir. Ölçekleme faktörü, arşivlenmiş güneş lekesi verilerimizden kaldırılmıştır, bu da gerçek fiziksel birimleri yansıtmaktadır.
Solar-Jeofizik Aktivite Raporu 2003 Jun 20 2200 UTC
NOAA © SWPC tarafından hazırlanmış ve SpaceWeatherLive.com tarafından işlenmiştir.USAF/NOAA Ortak Güneş ve Jeofizik Aktivite Raporu
SDF Numarası 171, 20 Jun 2003 üzerinden 2200Z'de Verildi
IA. 19-2100Z'den 20-2100Z'ye Solar Aktif Bölgelerin ve Aktivitenin Analizi
Solar activity increased to low levels today. Region
386 (S07E17) produced two low levels C-class flares today along with
several B-class flares. The northern portion of the penumbral field
appears to have undergone some rotation since yesterday while the
delta magnetic structure in the southern leading edge of group has
changed little during the period and remains intact. Region 387
(N18E36) was quiescent today although spot coverage and magnetic
complexity have both shown growth over the period. Region 389
(S12E14) was newly numbered today.
IB. Güneş Aktivitesi Tahmini
Solar activity is expected to range
from low to moderate levels. Region 386 remains capable of
producing an isolated major event.
IIA. Jeofiziksel Aktivite Özeti 19-2100Z ila 20-2100Z
The geomagnetic field was at predominantly unsettled levels today as
effects from the western most recurrent coronal hole wanes. The
greater than 2 MeV electron flux at geosynchronous orbit reached
high levels today.
IIB. Jeofiziksel Aktivite Tahmini
The geomagnetic field is
expected to be at predominantly unsettled levels. Active conditions
may exist especially at high latitudes beginning late on day two
with the return of a recurrent coronal hole high speed stream.
III. Olay Olasılıkları 21 Jun ila 23 Jun
| M Sınıfı | 40% | 40% | 40% |
| X Sınıfı | 10% | 10% | 10% |
| Proton | 10% | 10% | 10% |
| PCAF | yellow
|
IV. Penticton 10.7 cm Akı
Gözlemlendi 20 Jun 117
Tahmin edildi 21 Jun-23 Jun 115/115/120
90 Günlük Ortalama 20 Jun 125
V. Jeomanyetik A Endeksi
Gözlemlendi Afr/Ap 19 Jun 016/018
Tahmini Afr/Ap 20 Jun 010/015
Tahmin edildi Afr/Ap 21 Jun-23 Jun 010/015-012/015-012/020
VI. Jeomanyetik Aktivite Olasılıkları 21 Jun ila 23 Jun
| A. Orta Enlemler |
| Aktif | 15% | 25% | 25% |
| Küçük fırtına | 05% | 05% | 10% |
| Büyük-şiddetli fırtına | 01% | 01% | 01% |
| B. Yüksek Enlemler |
| Aktif | 30% | 30% | 40% |
| Küçük fırtına | 15% | 15% | 20% |
| Büyük-şiddetli fırtına | 05% | 05% | 05% |
99999
PLAIN
K-Indices:
On 16 June, it was determined that a scaling problem exists with the Boulder magnetometer instrument. While this problem, and its fix are being investigated the primary instrument for Boulder K-indices has been switched to the Boulder USGS (via Domsat) magnetometer, effective 1500 UTC on 16 June.
GOES Protons:
To ensure continued operational monitoring of important energetic particle data, it is necessary to reassign primary/secondary designations for the GOES Space Environment Monitor (SEM) detectors. GOES 11 (113W) is now the primary satellite for protons. GOES 12 will continue as the primary satellite for magnetometer, X-ray, and electron measurements. GOES 10 (135W) will be the secondary satellite for all SEM sensors - magnetometer, X-ray, and energetic particles. Because of the degraded state of the proton data on GOES-10, its designation as the secondary source for proton data is a short-term solution. More permanent solutions have been identified and are being evaluated. Users will be notified when we define and schedule a permanent fix. Further details can be found at http://www.sec.noaa.gov/GOES.html.
99999
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