Publié: 2018 Jul 16 1250 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 16 Jul 2018 | 073 | 012 |
| 17 Jul 2018 | 072 | 006 |
| 18 Jul 2018 | 071 | 007 |
During last 24 hours solar activity was very low with only two B-class flares reported. As the visible side of the solar disc is presently spotless we do not expect flaring activity in the coming hours. Presently available coronagraph images do not show signatures of the Earth directed CMEs, and the solar protons are at the background level. The in situ observations indicate arrival of the structure in the slow solar wind, of presently unclear solar origin. Early this morning interplanetary magnetic field started to increased (it reached the value of about 10 nT) following, with of about 10 hours of the delay, the increase of the density and drop of the temperature. The solar wind speed reached its maximum value (during last 24 hours) of about 340 km/s early this morning. The present value of the solar wind speed is 320 km/s and the interplanetary magnetic field magnitude is about 8 nT. Very patchy equatorial coronal hole, which seem to be connected to the low latitude extension of the northern polar coronal hole, has reached central meridian this morning. The increase of the solar wind speed, associated with this coronal hole is expected late on July 19. Due to longer interval of the negative value of the Bz component of the interplanetary magnetic field (down to -8 nT) local station at Dourbes reported disturbed geomagnetic conditions at about 09 UT today (K=4), and NOAA reported value of the Kp=3. The geomagnetic conditions are presently quiet to unsettled, and we expect quiet geomagnetic conditions to persist in the coming hours.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 000, sur la base de 27 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 072 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 005 |
| Ap estimé | 003 |
| Nombre international de taches solaires estimé | 000 - Basé sur 20 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio | |
|---|---|---|---|---|---|---|---|---|---|---|
| Aucun | ||||||||||
Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive
Toutes les heures sont indiquées en UTC
A lot of people come to SpaceWeatherLive to follow the Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!
| Dernière classe X | 18/01/2026 | X1.9 |
| Dernière classe M | 21/01/2026 | M3.4 |
| Dernier orage géomagnétique | 22/01/2026 | Kp5+ (G1) |
| Jours sans taches solaires | |
|---|---|
| Dernier jour sans taches solaires | 08/06/2022 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| décembre 2025 | 124 +32.2 |
| janvier 2026 | 117.9 -6.1 |
| 30 derniers jours | 121.2 +12.1 |