强耀斑一定会带来极光吗?
不一定。耀斑不等于朝向地球的日冕物质抛射;极光还取决于抵达地球的太阳风、磁场方向、观测位置、黑夜与天气。
今天太阳活跃吗?查看太阳耀斑、地磁暴和太阳风的最新观测,再结合所在城市的极光预报判断观测机会。
Bt 表示磁场总强度。Bz 持续为负,说明磁场朝南,更有利于太阳风能量进入地球磁场环境,但不保证一定能看到极光。
Kp 从 0 到 9,达到 5 才进入地磁暴分级。它反映全球磁场活动,不是某个城市看到极光的概率。
:Product: 3-Day Forecast
:Issued: 2026 Nov 02 0030 UTC
# Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center
#
A. NOAA Geomagnetic Activity Observation and Forecast
The greatest observed 3 hr Kp over the past 24 hours was 5 (NOAA Scale
G1).
The greatest expected 3 hr Kp for Nov 02-Nov 04 2026 is 3.00 (below NOAA
Scale levels).
NOAA Kp index breakdown Nov 02-Nov 04 2026
Nov 02 Nov 03 Nov 04
00-03UT 2.67 1.67 1.67
03-06UT 3.00 2.00 2.00
06-09UT 3.00 1.67 1.67
09-12UT 2.67 1.33 1.33
12-15UT 2.00 0.67 1.33
15-18UT 2.00 0.67 0.67
18-21UT 1.67 1.67 0.67
21-00UT 2.00 1.33 1.67
Rationale: No G1 (Minor) or greater geomagnetic storms are expected. No
significant transient or recurrent solar wind features are forecast.
B. NOAA Solar Radiation Activity Observation and Forecast
Solar radiation, as observed by NOAA GOES-18 over the past 24 hours, was
below S-scale storm level thresholds.
Solar Radiation Storm Forecast for Nov 02-Nov 04 2026
Nov 02 Nov 03 Nov 04
S1 or greater 1% 1% 1%
Rationale: No S1 (Minor) or greater solar radiation storms are expected.
No significant active region activity favorable for radiation storm
production is forecast.
C. NOAA Radio Blackout Activity and Forecast
No radio blackouts were observed over the past 24 hours.
Radio Blackout Forecast for Nov 02-Nov 04 2026
Nov 02 Nov 03 Nov 04
R1-R2 1% 1% 1%
R3 or greater 1% 1% 1%
Rationale: No R1 (Minor) or greater radio blackouts are expected. No
significant active region flare activity is forecast.
:Product: Forecast Discussion
:Issued: 2026 Nov 02 0030 UTC
# Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center
#
Solar Activity
.24 hr Summary...
Solar activity was at low levels. Region 4564 (N04E29, Cro/beta)
produced an impulsive C1.1 flare at 01/1236 UTC, the strongest of the
period. The region was in a phase of gradual decay over the past 24
hours.
Other activity included eruptive activity along a filament channel in
the NW quadrant beginning after ~01/1500 UTC. Subsequent SOHO/LASCO C2
coronagraph imagery contained a slow-moving CME signature beginning at
01/1848 UTC. Additional imagery is needed to analyze the event for any
Earth-directed components.
.Forecast...
Solar activity is expected to be at very low levels with a chance for
isolated C-class flares through 04 Nov.
Energetic Particle
.24 hr Summary...
The greater than 2 MeV electron flux reached high levels with a peak
flux of 5350pfu observed at 01/1550 UTC. The greater than 10 MeV proton
flux remained steady at background levels.
.Forecast...
The greater than 2 MeV electron flux is expected to continue at high
levels through 04 Nov. The greater than 10 MeV proton flux is expected
to continue at background levels through 04 Nov.
Solar Wind
.24 hr Summary...
Solar wind parameters reflected the continued influence of a positive
polarity CH HSS. Total magnetic field strength gradually declined from a
peak of 9 nT to ~5 Bt at the end of the UT day. The Bz component reached
a brief maximum southward deflection of -7 nT early in the period. Solar
wind speeds gradually declined from ~575 km/s to ~460 km/s over the past
24 hours. Phi angle transitioned from mostly positive to variable after
01/0742 UTC.
.Forecast...
Enhanced solar wind conditions are likely to continue through 02 Nov due
to waning positive polarity CH HSS influence. A return to mostly nominal
conditions is expected over 03-04 Nov.
Geospace
.24 hr Summary...
The geomagnetic field reached G1 (Minor) storm levels early in the
period due to positive polarity CH HSS influences.
.Forecast...
The geomagnetic field is likely to reach unsettled levels on 02 Nov,
with mostly quiet conditions likely on 03-04 Nov, as CH HSS influence
wanes.
:Product: 27-day Space Weather Outlook Table 27DO.txt
:Issued: 2026 Nov 02 0218 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC contact on the Web
# https://www.swpc.noaa.gov/content/subscription-services
#
# 27-day Space Weather Outlook Table
# Issued 2026-11-02
#
# UTC Radio Flux Planetary Largest
# Date 10.7 cm A Index Kp Index
2026 Nov 02 95 10 3
2026 Nov 03 100 5 2
2026 Nov 04 100 5 2
2026 Nov 05 105 10 3
2026 Nov 06 110 10 3
2026 Nov 07 115 10 3
2026 Nov 08 115 5 2
2026 Nov 09 120 15 4
2026 Nov 10 115 10 3
2026 Nov 11 110 10 3
2026 Nov 12 110 10 3
2026 Nov 13 105 5 2
2026 Nov 14 105 5 2
2026 Nov 15 105 5 2
2026 Nov 16 100 10 3
2026 Nov 17 95 20 5
2026 Nov 18 95 20 5
2026 Nov 19 90 10 3
2026 Nov 20 90 5 2
2026 Nov 21 85 5 2
2026 Nov 22 85 5 2
2026 Nov 23 85 5 2
2026 Nov 24 90 5 2
2026 Nov 25 95 5 2
2026 Nov 26 95 10 3
2026 Nov 27 95 24 5
2026 Nov 28 95 20 5
:Product: Summary of Space Weather Observations dayobs.txt
:Issued: 2026 Nov 02 0030 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC contact on the Web
# https://www.swpc.noaa.gov/content/subscription-services
#
# Summary of Space Weather Observations
#
:Solar_Region_Summary: 2026 Nov 01
# Region Location Sunspot Characteristics
# Helio Spot Spot Mag.
# Num Lat.,CMD Long. Area Extent class count class
4564 N04E29 203 20 8 CRO 9 B
4565 N14E47 184 40 2 HSX 1 A
太阳活动及其引发的近地空间环境变化。太阳耀斑、高能粒子和地磁暴是不同现象,不能混为一谈。
不一定。耀斑不等于朝向地球的日冕物质抛射;极光还取决于抵达地球的太阳风、磁场方向、观测位置、黑夜与天气。
公开科学观测与预报可能延迟或修订。预报不保证能看到极光,也不构成运行安全保证;涉及重要决策请遵循官方指引。