Arşiv Cumartesi, 8 Eylül 2018 görüntüleniyor

SIDC'den güneş ve jeomanyetik aktivite hakkında günlük bülten

Yayınlandı: 2018 Sep 08 1230 UTC

SIDC Tahmini

Güneş patlamaları

Quiet conditions (<50% probability of C-class flares)

Jeomanyetizma

Quiet (A<20 and K<4)

Güneş protonları

Quiet

	10cm akı	Ap
08 Sep 2018	069	006
09 Sep 2018	069	005
10 Sep 2018	069	005

Bülten

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.

Bugünün tahmini uluslararası güneş lekesi sayısı (ISN): 1 Tahmini gunes lekesi sayisi, 2 Istasyon sayisi.

07 Sep 2018 için güneş endeksleri

Kurt numarası Catania	000
10cm güneş akısı	068
AK Chambon La Forêt	006
AK Wingst	006
Tahmini Ap	005
Tahmini uluslararası güneş lekesi sayısı	000 - 36 istasyonlarına göre

Dikkat çeken olayların özeti

Güneş Etkileri Veri Analiz Merkezi tarafından sağlanmıştır© - SIDC - SpaceWeatherLive tarafından işlendi

SIDC'den güneş ve jeomanyetik aktivite hakkında günlük bülten

Yayınlandı: 2018 Sep 08 2104 UTC

SIDC Tahmini

Güneş patlamaları

Quiet conditions (<50% probability of C-class flares)

Jeomanyetizma

Quiet (A<20 and K<4)

Güneş protonları

Quiet

	10cm akı	Ap
08 Sep 2018	069	006
09 Sep 2018	069	005
10 Sep 2018	069	005

Bülten

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.

Bugünün tahmini uluslararası güneş lekesi sayısı (ISN): 1 Tahmini gunes lekesi sayisi, 2 Istasyon sayisi.

07 Sep 2018 için güneş endeksleri

Kurt numarası Catania	000
10cm güneş akısı	068
AK Chambon La Forêt	006
AK Wingst	006
Tahmini Ap	005
Tahmini uluslararası güneş lekesi sayısı	000 - 36 istasyonlarına göre

Dikkat çeken olayların özeti

Güneş Etkileri Veri Analiz Merkezi tarafından sağlanmıştır© - SIDC - SpaceWeatherLive tarafından işlendi

SIDC'den güneş ve jeomanyetik aktivite hakkında günlük bülten

Yayınlandı: 2018 Sep 08 2117 UTC

SIDC Tahmini

Güneş patlamaları

Quiet conditions (<50% probability of C-class flares)

Jeomanyetizma

Quiet (A<20 and K<4)

Güneş protonları

Quiet

	10cm akı	Ap
08 Sep 2018	069	006
09 Sep 2018	069	005
10 Sep 2018	069	005

Bülten

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.

Bugünün tahmini uluslararası güneş lekesi sayısı (ISN): 1 Tahmini gunes lekesi sayisi, 2 Istasyon sayisi.

07 Sep 2018 için güneş endeksleri

Kurt numarası Catania	000
10cm güneş akısı	068
AK Chambon La Forêt	006
AK Wingst	006
Tahmini Ap	005
Tahmini uluslararası güneş lekesi sayısı	000 - 36 istasyonlarına göre

Dikkat çeken olayların özeti

Güneş Etkileri Veri Analiz Merkezi tarafından sağlanmıştır© - SIDC - SpaceWeatherLive tarafından işlendi

SIDC'den güneş ve jeomanyetik aktivite hakkında günlük bülten

Yayınlandı: 2018 Sep 08 2118 UTC

SIDC Tahmini

Güneş patlamaları

Quiet conditions (<50% probability of C-class flares)

Jeomanyetizma

Quiet (A<20 and K<4)

Güneş protonları

Quiet

	10cm akı	Ap
08 Sep 2018	069	006
09 Sep 2018	069	005
10 Sep 2018	069	005

Bülten

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.

Bugünün tahmini uluslararası güneş lekesi sayısı (ISN): 1 Tahmini gunes lekesi sayisi, 2 Istasyon sayisi.

07 Sep 2018 için güneş endeksleri

Kurt numarası Catania	000
10cm güneş akısı	068
AK Chambon La Forêt	006
AK Wingst	006
Tahmini Ap	005
Tahmini uluslararası güneş lekesi sayısı	000 - 36 istasyonlarına göre

Dikkat çeken olayların özeti

Güneş Etkileri Veri Analiz Merkezi tarafından sağlanmıştır© - SIDC - SpaceWeatherLive tarafından işlendi

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