Випущено: 2014 Oct 23 1257 UTC
Major flares expected (X-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Warning condition (activity levels expected to increase, but no numeric forecast given)
10cm flux | Ap | |
---|---|---|
23 Oct 2014 | 221 | 012 |
24 Oct 2014 | 226 | 012 |
25 Oct 2014 | 231 | 011 |
During the past 24 hours, Catania sunspot group 88 (NOAA AR 2192) produced an X1.6 flare (peaking yesterday at 14:28 UT) and an M1.1 flare (peaking today at 09:50 UT). These flares were not associated with CMEs. Catania sunspot group 93 (NOAA AR 2195) close to the east solar limb produced an M1.4 flare peaking at 15:57 UT, and this flare was associated only with a narrow CME. Catania sunspot group 88 will remain the main flare source as it continues to grow (this is the largest sunspot group during the two solar cycles) and maintains the beta-gamma-delta configuration of its photospheric magnetic field. Although the sunspots of the main magnetic polarities are somewhat separating, we still expect the flaring activity up to X-level from this sunspot group. As the Catania sunspot group 88 is currently situated at the solar central meridian, a major eruption in this active region may lead to a geoeffective CME and a proton event. The Earth is currently inside a slow (around 430 km/s) solar wind flow with average (around 5 nT) interplanetary magnetic field (IMF) magnitude. The geomagnetic conditions are quiet and are expected to remain so. Yesterday an interval of K = 5 was reported by IZMIRAN and an interval of K = 4 by Dourbes (K index according to NOAA remained at the quiet to unsettled levels with K < 4). This interval of slightly disturbed geomagnetic conditions was produced by a slow solar wind interval with predominantly negative north-south IMF component Bz.
Today's estimated international sunspot number (ISN): 091, based on 05 stations.
Wolf number Catania | 202 |
10cm solar flux | 216 |
AK Chambon La Forêt | /// |
AK Wingst | /// |
Estimated Ap | 017 |
Estimated international sunspot number | 098 - Based on 16 stations |
Day | Begin | Max | Кінець | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types |
---|---|---|---|---|---|---|---|---|---|
22 | 1402 | 1428 | 1450 | S14E13 | X1.6 | 2B | 200 | 88/2192 | |
22 | 1551 | 1557 | 1603 | ---- | M1.4 | --/---- | II/1 | ||
23 | 0944 | 0950 | 0956 | S16E03 | M1.1 | 1F | 88/2192 |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
Весь час у UTC
Багато людей відвідують сайт SpaceWeatherLive, щоб слідкувати за сонячною та авроральною активністю, але зі збільшенням трафіку хостинг також стає дорожчим. Будь-ласка, подумайте про пожертву, якщо вам подобається SpaceWeatherLive, щоб ми могли і надалі підтримувати цей сайт і платити за хостинг!
Останній X-спалах | 2025/03/28 | X1.1 |
Останній M-спалах | 2025/04/01 | M5.6 |
Останній геомагнітний шторм | 2025/03/27 | Kp5 (G1) |
Дні без сонячних плям | |
---|---|
Останній день без сонячних спалахів | 2022/06/08 |
Середня кількість сонячних плям протягом місяця | |
---|---|
лютого 2025 | 154.6 +17.6 |
Останні 30 днів | 128.5 -22.7 |