Archiv von Samstag, 8 September 2018 anzeigen
Tägliches Bulletin zur solaren und geomagnetischen Aktivität des SIDC
Ausgestellt: 2018 Sep 08 1230 UTC
Vorhersage des SIDC
Sonneneruptionen
Quiet conditions (<50% probability of C-class flares)
Geomagnetismus
Quiet (A<20 and K<4)
Sonnenprotonen
Quiet
| 10cm Fluss | Ap | |
|---|---|---|
| 08 Sep 2018 | 069 | 006 |
| 09 Sep 2018 | 069 | 005 |
| 10 Sep 2018 | 069 | 005 |
Bulletin
Solar activity was at very low levels. A small sunspot region (NOAA 2721) developed early on 08 September near the disk's center. No earth-directed coronal mass ejections (CMEs) were observed in the available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal levels. A trans-equatorial positive polarity coronal hole (CH) has nearly finished its transit over the Central Meridian.
Solar activity is expected to remain at very low levels.
Solar wind speed declined from 520 to 360 km/s (DSCOVR). Bz varied between -3 and +3 nT, with a brief excursion to +6 nT around 07:30UT. The interplanetary magnetic field was directed towards the Sun (negative sector), turning into a positive sector after 10UT.
Quiet geomagnetic conditions were observed, with Kp recording an isolated unsettled episode during the 06-09UT interval. Mostly quiet geomagnetic conditions are expected with a chance on an unsettled episode until the arrival of the co-rotating interaction region (CIR) and wind stream from the positive polarity CH, most likely on 11 September.
Die heute international geschätzte Sonnenfleckenanzahl (ISN): 015, basierend auf 14 Stationen.Solarindizes für den 07 Sep 2018
| Wolf-Zahl Catania | 000 |
| 10cm Solarflux | 068 |
| AK Chambon La Forêt | 006 |
| AK Wingst | 006 |
| Geschätzer Ap-Wert | 005 |
| Geschätzte internationale Sonnenfleckenzahl | 000 - Basierend auf 36 Stationen |
Zusammenfassung auffälliger Ereignisse
| Tag | Start | Max | Ende | Loc | Stärke | OP | 10cm | Catania/NOAA | Radioburst-Typen | |
|---|---|---|---|---|---|---|---|---|---|---|
| Keine | ||||||||||
Zur Verfügung gestellt vom Solar Influences Data Analysis Center© - SIDC - Verarbeitet von SpaceWeatherLive
Tägliches Bulletin zur solaren und geomagnetischen Aktivität des SIDC
Ausgestellt: 2018 Sep 08 2104 UTC
Vorhersage des SIDC
Sonneneruptionen
Quiet conditions (<50% probability of C-class flares)
Geomagnetismus
Quiet (A<20 and K<4)
Sonnenprotonen
Quiet
| 10cm Fluss | Ap | |
|---|---|---|
| 08 Sep 2018 | 069 | 006 |
| 09 Sep 2018 | 069 | 005 |
| 10 Sep 2018 | 069 | 005 |
Bulletin
Solar activity was at very low levels. A small sunspot region (NOAA 2721) developed early on 08 September near the disk's center. No earth-directed coronal mass ejections (CMEs) were observed in the available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal levels. A trans-equatorial positive polarity coronal hole (CH) has nearly finished its transit over the Central Meridian.
Solar activity is expected to remain at very low levels.
Solar wind speed declined from 520 to 360 km/s (DSCOVR). Bz varied between -3 and +3 nT, with a brief excursion to +6 nT around 07:30UT. The interplanetary magnetic field was directed towards the Sun (negative sector), turning into a positive sector after 10UT.
Quiet geomagnetic conditions were observed, with Kp recording an isolated unsettled episode during the 06-09UT interval. Mostly quiet geomagnetic conditions are expected with a chance on an unsettled episode until the arrival of the co-rotating interaction region (CIR) and wind stream from the positive polarity CH, most likely on 11 September.
Die heute international geschätzte Sonnenfleckenanzahl (ISN): 015, basierend auf 14 Stationen.Solarindizes für den 07 Sep 2018
| Wolf-Zahl Catania | 000 |
| 10cm Solarflux | 068 |
| AK Chambon La Forêt | 006 |
| AK Wingst | 006 |
| Geschätzer Ap-Wert | 005 |
| Geschätzte internationale Sonnenfleckenzahl | 000 - Basierend auf 36 Stationen |
Zusammenfassung auffälliger Ereignisse
| Tag | Start | Max | Ende | Loc | Stärke | OP | 10cm | Catania/NOAA | Radioburst-Typen | |
|---|---|---|---|---|---|---|---|---|---|---|
| Keine | ||||||||||
Zur Verfügung gestellt vom Solar Influences Data Analysis Center© - SIDC - Verarbeitet von SpaceWeatherLive
Tägliches Bulletin zur solaren und geomagnetischen Aktivität des SIDC
Ausgestellt: 2018 Sep 08 2117 UTC
Vorhersage des SIDC
Sonneneruptionen
Quiet conditions (<50% probability of C-class flares)
Geomagnetismus
Quiet (A<20 and K<4)
Sonnenprotonen
Quiet
| 10cm Fluss | Ap | |
|---|---|---|
| 08 Sep 2018 | 069 | 006 |
| 09 Sep 2018 | 069 | 005 |
| 10 Sep 2018 | 069 | 005 |
Bulletin
Solar activity was at very low levels. A small sunspot region (NOAA 2721) developed early on 08 September near the disk's center. No earth-directed coronal mass ejections (CMEs) were observed in the available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal levels. A trans-equatorial positive polarity coronal hole (CH) has nearly finished its transit over the Central Meridian.
Solar activity is expected to remain at very low levels.
Solar wind speed declined from 520 to 360 km/s (DSCOVR). Bz varied between -3 and +3 nT, with a brief excursion to +6 nT around 07:30UT. The interplanetary magnetic field was directed towards the Sun (negative sector), turning into a positive sector after 10UT.
Quiet geomagnetic conditions were observed, with Kp recording an isolated unsettled episode during the 06-09UT interval. Mostly quiet geomagnetic conditions are expected with a chance on an unsettled episode until the arrival of the co-rotating interaction region (CIR) and wind stream from the positive polarity CH, most likely on 11 September.
Die heute international geschätzte Sonnenfleckenanzahl (ISN): 015, basierend auf 14 Stationen.Solarindizes für den 07 Sep 2018
| Wolf-Zahl Catania | 000 |
| 10cm Solarflux | 068 |
| AK Chambon La Forêt | 006 |
| AK Wingst | 006 |
| Geschätzer Ap-Wert | 005 |
| Geschätzte internationale Sonnenfleckenzahl | 000 - Basierend auf 36 Stationen |
Zusammenfassung auffälliger Ereignisse
| Tag | Start | Max | Ende | Loc | Stärke | OP | 10cm | Catania/NOAA | Radioburst-Typen | |
|---|---|---|---|---|---|---|---|---|---|---|
| Keine | ||||||||||
Zur Verfügung gestellt vom Solar Influences Data Analysis Center© - SIDC - Verarbeitet von SpaceWeatherLive
Tägliches Bulletin zur solaren und geomagnetischen Aktivität des SIDC
Ausgestellt: 2018 Sep 08 2118 UTC
Vorhersage des SIDC
Sonneneruptionen
Quiet conditions (<50% probability of C-class flares)
Geomagnetismus
Quiet (A<20 and K<4)
Sonnenprotonen
Quiet
| 10cm Fluss | Ap | |
|---|---|---|
| 08 Sep 2018 | 069 | 006 |
| 09 Sep 2018 | 069 | 005 |
| 10 Sep 2018 | 069 | 005 |
Bulletin
Solar activity was at very low levels. A small sunspot region (NOAA 2721) developed early on 08 September near the disk's center. No earth-directed coronal mass ejections (CMEs) were observed in the available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal levels. A trans-equatorial positive polarity coronal hole (CH) has nearly finished its transit over the Central Meridian.
Solar activity is expected to remain at very low levels.
Solar wind speed declined from 520 to 360 km/s (DSCOVR). Bz varied between -3 and +3 nT, with a brief excursion to +6 nT around 07:30UT. The interplanetary magnetic field was directed towards the Sun (negative sector), turning into a positive sector after 10UT.
Quiet geomagnetic conditions were observed, with Kp recording an isolated unsettled episode during the 06-09UT interval. Mostly quiet geomagnetic conditions are expected with a chance on an unsettled episode until the arrival of the co-rotating interaction region (CIR) and wind stream from the positive polarity CH, most likely on 11 September.
Die heute international geschätzte Sonnenfleckenanzahl (ISN): 015, basierend auf 14 Stationen.Solarindizes für den 07 Sep 2018
| Wolf-Zahl Catania | 000 |
| 10cm Solarflux | 068 |
| AK Chambon La Forêt | 006 |
| AK Wingst | 006 |
| Geschätzer Ap-Wert | 005 |
| Geschätzte internationale Sonnenfleckenzahl | 000 - Basierend auf 36 Stationen |
Zusammenfassung auffälliger Ereignisse
| Tag | Start | Max | Ende | Loc | Stärke | OP | 10cm | Catania/NOAA | Radioburst-Typen | |
|---|---|---|---|---|---|---|---|---|---|---|
| Keine | ||||||||||
Zur Verfügung gestellt vom Solar Influences Data Analysis Center© - SIDC - Verarbeitet von SpaceWeatherLive
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