SWERTO_SERVICES

NOWCASTING

GOES Proton Flux
DASHBOARD_PAMELA
GOES X-ray Flux
DASHBOARD_GOESX

FORECASTING

M-class Flare
DASHBOARD_RP
X-class Flare
DASHBOARD_CME
SPE Peak Fluxes
DASHBOARD_SPE

PROGETTO

DESCRIZIONE_PROGETTO

PAMELA

DESCRIZIONE_PAMELA


ALTEA

ALTEA_PAR_1



Figura 2: A sinistra: configurazione di ALTEA “a caschetto”. A destra, l’astronauta statunitense Sunita Wiliams che indossa il caschetto durante una seduta di misura ALTEA
Figura 3: Configurazione SURVEY di ALTEA, con i tre telescopi lungo i tre assi cartesiani (X,Y,Z).
Figura 4: Configurazione ALTEA-Shield. In arancione è possibile notare le tiles di materiale su due delle tre SDU.

ALTEA_PAR_1_IMG


IBIS

DESCRIZIONE_IBIS

Timetable of IBIS datasets available, with target and status of the data. If you are interested in any of these datasets, please contact spaceweather@roma2.infn.it
Year days Spectral Lines and Stokes parameters State Target FoV position Overall Quality
2003 Oct 16 FeI 709.0 I FeII 722.4 I CaII 854.2 I RAW: NA RED:10GB Quiet Sun Disk Centre HIGH
2005 Sep 28 FeI 709.0 I FeII 722.4 I CaII 854.2 I RAW: 105GB RED:54GB AR 10812 Disk Centre HIGH
2006 Nov 21 FeI 630.1 I+Q+U+V FeI 630.2 I+Q+U+V CaII 854.2 I+V RAW: 375GB RED:10GB Quiet Sun Disk Centre EXCELLENT
2007 Sep 14, 21, 22 FeI 630.2 I+Q+U+V RAW: 295GB RED:--- Quiet Sun Disk Centre, centre to limb LOW
2007 Nov 13, 15, 17, 18, 19 NiI 676.9 I FeI 709.0 I CaII 854.2 I RAW: 670GB RED:52GB Quiet Sun, unnamed AR Disk Centre, limb LOW
2008 Oct 13, 15, 16, 18, 19, 20 FeI 617.3 I+Q+U+V CaII 854.2 I RAW: 335GB RED:35GB Quiet Sun, unnamed AR Disk Centre, limb MEDIUM, HIGH on 15
2010 Oct 2, 7, 8, 9 FeI 617.3 I+Q+U+V CaII 854.2 I+Q+U+V RAW: 680GB RED:--- AR 1111 on 2,Quiet Sun, AR 1112 on 9 Disk Centre, limb LOW, MEDIUM on 9
2013 Jan 19, Feb 14 FeI 617.3 I+Q+U+V CaII 854.2 I+Q+U+V RAW: 1400GB RED:100GB Quiet Sun Limb MEDIUM

MOTH

DESCRIZIONE_MOTH

Timetable of MOTH datasets available, with status of the data. If you are interested in any of these datasets, please contact spaceweather@roma2.infn.it
Year days Spectral Lines State FoV Overall Quality
2014 Jun 29,30 K I 770 nm, Na D2 589 nm RAW: 66GB RED: --- Full Disk low
2014 Jul 1 K I 770 nm, Na D2 589 nm RAW: 35GB RED: --- Full Disk low
2014 Jul 2,3,8,9,11,23 K I 770 nm, Na D2 589 nm RAW: 630GB RED: 63GB Full Disk high
2014 Aug 3 K I 770 nm, Na D2 589 nm RAW: 120GB RED: --- Full Disk low
2015 Dec 23 K I 770 nm, Na D2 589 nm RAW: 90GB RED: --- Full Disk low
2017 Jan 21,22 K I 770 nm, Na D2 589 nm RAW: 5TB RED: 650GB Full Disk medium
2017 Jan 23,24,25 K I 770 nm, Na D2 589 nm RAW: 8TB RED: 1TB Full Disk medium

CASI_STUDIO

CASI_STUDIO_PAR_1


CASI_STUDIO_PAR_2

Figura 1: The energy loss spectrum of the May 17th, 2012 SPE (as seen on board the ISS by ALTEA detector), integrated over the polar passages, is shown in comparison with a reference period of quiet sun (April 20th–May 16th). Both spectra are normalized by the effective time of detector acquisition, by the geometrical factor and by the energy loss unit.

Figura 2: Active regions AR11429 and AR11430 as observed by SDO imagers around the March 7th event: (a) SDO/HMI Continuum; (b) SDO/ HMI Magnetogram; (c) SDO/AIA 335 A ̊ ; [d] SDO/AIA 171 A ̊ .

CASI_STUDIO_PAR_3


CASI_STUDIO_PAR_4

Figura 3: GOES proton data (above) and ALTEA data below, during the December 13th, 2006 SPE. The different component and modulation of the ALTEA measurements are marked. On the bottom right a typical day in a quite period to enlarge the south - north poles asymmetry.

Figura 4: Proton and helium absolute fluxes as measured by PAMELA for the SEP event on 14 December 2006.

CASI_STUDIO_PAR_5


CASI_STUDIO_PAR_6

Figura 5: Time profile of the geomagnetic cutoff latitudes measured by PAMELA, for different rigidity bins (color code). The vertical lines mark the beginning of the storm initial, main and recovery phases, respectively.

Figura 6: (Top) PAMELA’s pitch angle distribution (background subtracted) in three rigidity ranges. The curves through the data are meant to guide the eye. Also shown is the world-wide neutron monitor pitch angle distribution averaged between 0158 and 0220 UT.

CASI_STUDIO_PAR_7

INDUSTRIE

INDUSTRIE_text

DIZIONARIO_SW

Dizionario_text

FAQ

FAQ_text

DISCLAIMER

DISCLAIMER_text