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  • Day's last
    GOES
    NONE
    R0

    R0

    Event date: N/A

    No available description!

    UNAVAIABLE
    NONE
    G0

    G0

    Event date: N/A

    No available description!

    UNAVAIABLE
    NONE
    S0

    S0

    Event date: N/A

    No available description!

  • Day's max
    GOES
    NONE
    R0

    R0

    Event date: N/A

    No available description!

    UNAVAIABLE
    NONE
    G0

    G0

    Event date: N/A

    No available description!

    UNAVAIABLE
    NONE
    S0

    S0

    Event date: N/A

    No available description!

  • Latest event
    GOES
    CLASS M
    R1

    R1

    Event date: 2025-05-14

    Sailing: navigation signal low frequency degraded for brief intervals.

    HF Radio: Weak or small degradation in HF communication in the lighted area of the Earth, occasional loss of radio contact.

    UNAVAIABLE
    NONE
    G0

    G0

    Event date: N/A

    No available description!

    UNAVAIABLE
    NONE
    S0

    S0

    Event date: N/A

    No available description!

  • 2025-05-11
    GOES
    NONE
    R0

    R0

    Event date: N/A

    No available description!

    UNAVAIABLE
    NONE
    G0

    G0

    Event date: N/A

    No available description!

    UNAVAIABLE
    NONE
    S0

    S0

    Event date: N/A

    No available description!

  • 2025-05-12
    GOES
    NONE
    R0

    R0

    Event date: N/A

    No available description!

    UNAVAIABLE
    NONE
    G0

    G0

    Event date: N/A

    No available description!

    UNAVAIABLE
    NONE
    S0

    S0

    Event date: N/A

    No available description!

  • 2025-05-13
    GOES
    CLASS X
    R3

    R3

    Event date: 2025-05-13

    Sailing: Navigating low frequency degraded for about an hour.

    HF Radio: Large area blackout in HF radio communication, loss of radio contact for about an hour in the illuminated region.

    UNAVAIABLE
    NONE
    G0

    G0

    Event date: N/A

    No available description!

    UNAVAIABLE
    NONE
    S0

    S0

    Event date: N/A

    No available description!

  • Yesterday, 2025-05-14
    GOES
    CLASS M
    R1

    R1

    Event date: 2025-05-14

    Sailing: navigation signal low frequency degraded for brief intervals.

    HF Radio: Weak or small degradation in HF communication in the lighted area of the Earth, occasional loss of radio contact.

    UNAVAIABLE
    NONE
    G0

    G0

    Event date: N/A

    No available description!

    UNAVAIABLE
    NONE
    S0

    S0

    Event date: N/A

    No available description!

Media

Category Archives: Public

MINUTE OF 138th BRIEFING: 04/05/2015, 14H30

Space Weather Exhibition Room/INPE-SJC SUN Forecaster 1: During the Last week (April 28th to May 4th) was observed two coronal holes. The first CH665 was geo-effective on May 02nd and the second was located over Southern Hemisphere. We observed a …

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Lívia Ribeiro Alves •7 de May de 2015Media, Public, Scientists

Global Plan to Protect the Society for Space Weather Effects

Author: Dr. Clezio Marcos De Nardin After 3 years of work, the final version of the Global Plan to protect the Society of Space Weather Effects (complete title: Understanding space weather to shield society: The global road map for 2015-2025 commissioned …

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Lívia Ribeiro Alves •4 de May de 2015Educators, Media, Public, Scientists

MINUTE OF 136th BRIEFING: 13/03/2015, 14H30

Space Weather Exhibition Room/INPE-SJC SUN Forecaster 1: During the last week (April 07th to 12th) it was recorded two M-class Flares. The first Flare was emitted by 2320 geo-effective region and the second Flare was emitted by 2321 region. This …

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Lívia Ribeiro Alves •16 de April de 2015Educators, Media, Public, Scientists

MINUTE OF 135th BRIEFING: 06/03/2015, 14H30

Space Weather Exhibition Room /INPE-SJC SUN Forecaster 1: During the last weak (March 31st to April 6th) were recorded some B and C-class Flares. We observed a trans-equatorial coronal hole (CH661) that was geo-effective from March 30th. A second coronal …

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Lívia Ribeiro Alves •7 de April de 2015Educators, Media, No Category, Public

MINUTE OF 134th BRIEFING: 30/03/2015, 14H30

Space Weather Exhibition Room/INPE-SJC SUN Forecaster 1: During the last week (March 24th to 30th), some C-class Flares were recorded, among them the most intense reached a C9 classification. We observed over Southern Hemisphere a coronal hole that was geo-effective …

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Lívia Ribeiro Alves •31 de March de 2015Educators, Media, Public, Scientists

MINUTE OF 133st BRIEFING: 23/03/2015, 14H30

Space Weather Exhibition Room /INPE-SJC SUN Forecaster 1: During the week between 17 to 23 March, were recorded 3 M-class Flares emitted from sunspot 12297. We observed a coronal hole (CH 660) on the solar disc southern hemisphere. This coronal …

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Lívia Ribeiro Alves •25 de March de 2015Educators, Media, Public, Scientists

Minute of the 131st Briefing March 9, 2015, 14H30

Space Weather exhibition room/INPE-SJC SUN Forecaster 1: The week between March 2nd-9st, were recorded at least 6 M-class Flares. These Flares were able to cause blackout in the radio frequencies. It was also observed a CME associated with M-class Flare …

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Lívia Ribeiro Alves •11 de March de 2015Media, Public, Scientists

The complexity of three solar Magi Kings

Authors: Rafael R. S. de Mendonça, Carlos R. Braga As well as the Three Magi Kings, three coronal mass ejections (CMEs) left their birthplace (the Sun) and passed the Earth during the last Christmas. The first CME (Melchior) was ejected on day …

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Lívia Ribeiro Alves •13 de February de 2015Educators, Public, Scientists

Brazilian space weather program signs cooperation agreement with China

November 2013, during the visit of Vice-President of the Republic of China on the occasion of the Third Meeting of the Sino-Brazilian Commission for Coordination and Cooperation High Level (High-level Committee) was signed by the Presidents of the Brazilian Space …

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Lívia Ribeiro Alves •30 de January de 2015Media, Public

Vast coronal holes are observed in the solar disk

Author: Msc. Marcia Guedes Coronal holes are regions of the solar corona where the magnetic field extends into the space in lines “open”, where particles escape leading to the solar wind. Once trapped in the closed magnetic field lines, the …

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Lívia Ribeiro Alves •30 de January de 2015Educators, Public
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