View in EDS

Sun CubE OnE: A multi-wavelength synoptic solar micro satellite.

Saved in:
Bibliographic Details
Title: Sun CubE OnE: A multi-wavelength synoptic solar micro satellite.
Authors: Giovannelli, L.1 (AUTHOR), Berrilli, F.1 (AUTHOR) francesco.berrilli@roma2.infn.it, Casolino, M.2 (AUTHOR), Curti, F.3 (AUTHOR), Del Moro, D.1 (AUTHOR), Calchetti, D.1 (AUTHOR), Cantoresi, M.1 (AUTHOR), D'Ambrosio, A.3 (AUTHOR), Francisco, G.1 (AUTHOR), Giobbi, P.1 (AUTHOR), Marcelli, L.2 (AUTHOR), Mazzotta, P.1 (AUTHOR), Mugatwala, R.1 (AUTHOR), Pucacco, G.1 (AUTHOR), Reda, R.1 (AUTHOR), Dhara, S.K.1 (AUTHOR), Tombesi, F.1 (AUTHOR), Blandino, D.4 (AUTHOR), Benigno, N.5 (AUTHOR), Cilia, M.4 (AUTHOR)
Source: Advances in Space Research. Feb2023, Vol. 71 Issue 4, p1995-2005. 11p.
Subjects: Microspacecraft, Space environment, Bremsstrahlung, Solar activity, Solar cycle, Solar oscillations, Geomagnetism, Solar flares
Abstract: The Sun cubE onE (SEE) is a 12U CubeSat mission proposed for a phase A/B study to the Italian Space Agency that will investigate Gamma and X-ray fluxes and ultraviolet (UV) solar emission to support studies in Sun-Earth interaction and Space Weather from LEO. More in detail, SEE's primary goals are to measure the flares emission from soft-X to Gamma ray energy range and to monitor the solar activity in the Fraunhofer Mg II doublet at 280 nm, taking advantage of a full disk imager payload. The Gamma and X-ray fluxes will be studied with unprecedented temporal resolution and with a multi-wavelength approach thanks to the combined use of silicon photodiode and silicon photomultiplier (SiPM) -based detectors. The flare spectrum will be explored from the keV to the MeV range of energies by the same payload, and with a cadence up to 10 kHz and with single-photon detection capabilities to unveil the sources of the solar flares. The energy range covers the same bands used by GOES satellites, which are the standard bands for flare magnitude definition. At the same time SiPM detectors combined with scintillators allow to cover the non-thermal bremsstrahlung emission in the gamma energy range. Given its UV imaging capabilities, SEE will be a key space asset to support detailed studies on solar activity, especially in relation to ultraviolet radiation which strongly interacts with the upper layers of the Earth's atmosphere, and in relation to space safety, included in the field of human space exploration. The main goal for the UV payload is to study the evolution of the solar UV emission in the Mg II band at two different time scales: yearly variations along the solar cycle and transient variations during flare events. The Mg II index is commonly used as a proxy of the solar activity in the Sun-as-a-star paradigm, in which solar irradiance variations in the UV correlate with the variations in stratospheric ozone concentrations and other physical parameters of the Earth high atmosphere. SEE data will be used together with space and ground-based observatories that provide Solar data (e.g. Solar Orbiter, IRIS, GONG, TSST), high energy particle fluxes (e.g. GOES, MAXI, CSES) and geomagnetic data in a multi-instrument/multi-wavelength/multi-messenger approach. [ABSTRACT FROM AUTHOR]
Copyright of Advances in Space Research is the property of Pergamon Press - An Imprint of Elsevier Science and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
Database: Engineering Source
FullText Text:
  Availability: 0
Header DbId: egs
DbLabel: Engineering Source
An: 161527245
AccessLevel: 6
PubType: Academic Journal
PubTypeId: academicJournal
PreciseRelevancyScore: 0
IllustrationInfo
Items – Name: Title
  Label: Title
  Group: Ti
  Data: Sun CubE OnE: A multi-wavelength synoptic solar micro satellite.
– Name: Author
  Label: Authors
  Group: Au
  Data: <searchLink fieldCode="AR" term="%22Giovannelli%2C+L%2E%22">Giovannelli, L.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Berrilli%2C+F%2E%22">Berrilli, F.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> francesco.berrilli@roma2.infn.it</i><br /><searchLink fieldCode="AR" term="%22Casolino%2C+M%2E%22">Casolino, M.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Curti%2C+F%2E%22">Curti, F.</searchLink><relatesTo>3</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Del+Moro%2C+D%2E%22">Del Moro, D.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Calchetti%2C+D%2E%22">Calchetti, D.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Cantoresi%2C+M%2E%22">Cantoresi, M.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22D'Ambrosio%2C+A%2E%22">D'Ambrosio, A.</searchLink><relatesTo>3</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Francisco%2C+G%2E%22">Francisco, G.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Giobbi%2C+P%2E%22">Giobbi, P.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Marcelli%2C+L%2E%22">Marcelli, L.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Mazzotta%2C+P%2E%22">Mazzotta, P.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Mugatwala%2C+R%2E%22">Mugatwala, R.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Pucacco%2C+G%2E%22">Pucacco, G.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Reda%2C+R%2E%22">Reda, R.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Dhara%2C+S%2EK%2E%22">Dhara, S.K.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Tombesi%2C+F%2E%22">Tombesi, F.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Blandino%2C+D%2E%22">Blandino, D.</searchLink><relatesTo>4</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Benigno%2C+N%2E%22">Benigno, N.</searchLink><relatesTo>5</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Cilia%2C+M%2E%22">Cilia, M.</searchLink><relatesTo>4</relatesTo> (AUTHOR)
– Name: TitleSource
  Label: Source
  Group: Src
  Data: <searchLink fieldCode="JN" term="%22Advances+in+Space+Research%22">Advances in Space Research</searchLink>. Feb2023, Vol. 71 Issue 4, p1995-2005. 11p.
– Name: Subject
  Label: Subjects
  Group: Su
  Data: <searchLink fieldCode="DE" term="%22Microspacecraft%22">Microspacecraft</searchLink><br /><searchLink fieldCode="DE" term="%22Space+environment%22">Space environment</searchLink><br /><searchLink fieldCode="DE" term="%22Bremsstrahlung%22">Bremsstrahlung</searchLink><br /><searchLink fieldCode="DE" term="%22Solar+activity%22">Solar activity</searchLink><br /><searchLink fieldCode="DE" term="%22Solar+cycle%22">Solar cycle</searchLink><br /><searchLink fieldCode="DE" term="%22Solar+oscillations%22">Solar oscillations</searchLink><br /><searchLink fieldCode="DE" term="%22Geomagnetism%22">Geomagnetism</searchLink><br /><searchLink fieldCode="DE" term="%22Solar+flares%22">Solar flares</searchLink>
– Name: Abstract
  Label: Abstract
  Group: Ab
  Data: The Sun cubE onE (SEE) is a 12U CubeSat mission proposed for a phase A/B study to the Italian Space Agency that will investigate Gamma and X-ray fluxes and ultraviolet (UV) solar emission to support studies in Sun-Earth interaction and Space Weather from LEO. More in detail, SEE's primary goals are to measure the flares emission from soft-X to Gamma ray energy range and to monitor the solar activity in the Fraunhofer Mg II doublet at 280 nm, taking advantage of a full disk imager payload. The Gamma and X-ray fluxes will be studied with unprecedented temporal resolution and with a multi-wavelength approach thanks to the combined use of silicon photodiode and silicon photomultiplier (SiPM) -based detectors. The flare spectrum will be explored from the keV to the MeV range of energies by the same payload, and with a cadence up to 10 kHz and with single-photon detection capabilities to unveil the sources of the solar flares. The energy range covers the same bands used by GOES satellites, which are the standard bands for flare magnitude definition. At the same time SiPM detectors combined with scintillators allow to cover the non-thermal bremsstrahlung emission in the gamma energy range. Given its UV imaging capabilities, SEE will be a key space asset to support detailed studies on solar activity, especially in relation to ultraviolet radiation which strongly interacts with the upper layers of the Earth's atmosphere, and in relation to space safety, included in the field of human space exploration. The main goal for the UV payload is to study the evolution of the solar UV emission in the Mg II band at two different time scales: yearly variations along the solar cycle and transient variations during flare events. The Mg II index is commonly used as a proxy of the solar activity in the Sun-as-a-star paradigm, in which solar irradiance variations in the UV correlate with the variations in stratospheric ozone concentrations and other physical parameters of the Earth high atmosphere. SEE data will be used together with space and ground-based observatories that provide Solar data (e.g. Solar Orbiter, IRIS, GONG, TSST), high energy particle fluxes (e.g. GOES, MAXI, CSES) and geomagnetic data in a multi-instrument/multi-wavelength/multi-messenger approach. [ABSTRACT FROM AUTHOR]
– Name: AbstractSuppliedCopyright
  Label:
  Group: Ab
  Data: <i>Copyright of Advances in Space Research is the property of Pergamon Press - An Imprint of Elsevier Science and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
PLink https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&db=egs&AN=161527245
RecordInfo BibRecord:
  BibEntity:
    Identifiers:
      – Type: doi
        Value: 10.1016/j.asr.2022.09.044
    Languages:
      – Code: eng
        Text: English
    PhysicalDescription:
      Pagination:
        PageCount: 11
        StartPage: 1995
    Subjects:
      – SubjectFull: Microspacecraft
        Type: general
      – SubjectFull: Space environment
        Type: general
      – SubjectFull: Bremsstrahlung
        Type: general
      – SubjectFull: Solar activity
        Type: general
      – SubjectFull: Solar cycle
        Type: general
      – SubjectFull: Solar oscillations
        Type: general
      – SubjectFull: Geomagnetism
        Type: general
      – SubjectFull: Solar flares
        Type: general
    Titles:
      – TitleFull: Sun CubE OnE: A multi-wavelength synoptic solar micro satellite.
        Type: main
  BibRelationships:
    HasContributorRelationships:
      – PersonEntity:
          Name:
            NameFull: Giovannelli, L.
      – PersonEntity:
          Name:
            NameFull: Berrilli, F.
      – PersonEntity:
          Name:
            NameFull: Casolino, M.
      – PersonEntity:
          Name:
            NameFull: Curti, F.
      – PersonEntity:
          Name:
            NameFull: Del Moro, D.
      – PersonEntity:
          Name:
            NameFull: Calchetti, D.
      – PersonEntity:
          Name:
            NameFull: Cantoresi, M.
      – PersonEntity:
          Name:
            NameFull: D'Ambrosio, A.
      – PersonEntity:
          Name:
            NameFull: Francisco, G.
      – PersonEntity:
          Name:
            NameFull: Giobbi, P.
      – PersonEntity:
          Name:
            NameFull: Marcelli, L.
      – PersonEntity:
          Name:
            NameFull: Mazzotta, P.
      – PersonEntity:
          Name:
            NameFull: Mugatwala, R.
      – PersonEntity:
          Name:
            NameFull: Pucacco, G.
      – PersonEntity:
          Name:
            NameFull: Reda, R.
      – PersonEntity:
          Name:
            NameFull: Dhara, S.K.
      – PersonEntity:
          Name:
            NameFull: Tombesi, F.
      – PersonEntity:
          Name:
            NameFull: Blandino, D.
      – PersonEntity:
          Name:
            NameFull: Benigno, N.
      – PersonEntity:
          Name:
            NameFull: Cilia, M.
    IsPartOfRelationships:
      – BibEntity:
          Dates:
            – D: 15
              M: 02
              Text: Feb2023
              Type: published
              Y: 2023
          Identifiers:
            – Type: issn-print
              Value: 02731177
          Numbering:
            – Type: volume
              Value: 71
            – Type: issue
              Value: 4
          Titles:
            – TitleFull: Advances in Space Research
              Type: main
ResultId 1