SPANISH CONTRIBUTION IN CRYOGENIC SPACE MISSIONS: DEVELOPMENTS FOR SPICA AND ATHENA, POST-OPERATIONS OF HERSCHEL AND MULTI-FREQUENCY SCIENTIFIC EXPLOITATION. (Q3137180): Difference between revisions
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(Created claim: summary (P836): In the last two decades, SPAIN has developed an important SCIENTIFIC AND TECHNICAL COMMUNITY IN INFRARROWING (IR) AND IN RATES X THAT WITH EXIT, AS CO-INVESTIGATOR, TO THE DEVELOPMENT AND SCIENTIFIC EXPLOTATION OF THE MAYORIA OF EUROPEAN SPACEMENTS._x000D_ _x000D_ The CAB sub-project Combines Expertise in CRIOGENIA TECHNOLOGY (A MK) and SPACIAL MECHANICAL WITH EXPERIENCE IN SCIENTIFIC EXPLOTATION IN MM/SUB/FAR-IR AND RAYS X, which would allow a...) |
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SPANISH CONTRIBUTION IN CRYOGENIC SPACE MISSIONS: DEVELOPMENTS FOR SPICA AND ATHENA, POST-OPERATIONS OF HERSCHEL AND MULTI-FREQUENCY SCIENTIFIC EXPLOITATION. | |||
Revision as of 13:52, 12 October 2021
Project Q3137180 in Spain
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | SPANISH CONTRIBUTION IN CRYOGENIC SPACE MISSIONS: DEVELOPMENTS FOR SPICA AND ATHENA, POST-OPERATIONS OF HERSCHEL AND MULTI-FREQUENCY SCIENTIFIC EXPLOITATION. |
Project Q3137180 in Spain |
Statements
278,300.0 Euro
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556,600.0 Euro
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50.0 percent
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1 January 2016
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30 June 2019
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AGENCIA CONSEJO SUPERIOR DE INVESTIGACIONES CIENTIFICAS
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40°27'31.61"N, 3°28'45.59"W
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28148
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EN LAS DOS ULTIMAS DECADAS, ESPAÑA HA DESARROLLADO UNA IMPORTANTE COMUNIDAD CIENTIFICA Y TECNICA EN EL INFRARROJO (IR) Y EN RAYOS X QUE HA CONTRIBUIDO CON EXITO, COMO CO-INVESTIGADOR, AL DESARROLLO Y EXPLOTACION CIENTIFICA DE LA MAYORIA DE INSTRUMENTOS EN MISIONES ESPACIALES EUROPEAS._x000D_ _x000D_ EL SUBPROYECTO DEL CAB COMBINA LA EXPERIENCIA EN TECNOLOGIA DE CRIOGENIA (A MK) Y MECANICA ESPACIAL CON LA EXPERIENCIA EN LA EXPLOTACION CIENTIFICA EN EL MM/SUB/FAR-IR Y RAYOS X, QUE PERMITIRA DAR UN SALTO CUANTITATIVO Y CUALITATIVO EN LA INVOLUCRACION ESPAÑOLA EN EL DISEÑO Y DESARROLLO DE INSTRUMENTACION ESPACIAL EN ESTOS RANGOS DE ENERGIA._x000D_ _x000D_ SE ACOMETE EL RETO DE CONTINUAR CO-LIDERANDO (CO-INVESTIGADOR PRINCIPAL -CO-IP-) EL DESARROLLO DEL INSTRUMENTO CRIOGENICO SAFARI EN EL IR MEDIO Y LEJANO DE LA MISION SPICA Y EL DESARROLLO DE DETECTORES SUPERCONDUCTORES. EN EL CASO DE LOS RAYOS X, EL CAB LIDERA (MIGUEL MAS ES XIFU CONSORTIUM BOARD MEMBER) LA DEFINICION Y CONSTRUCCION DEL CRIOSTATO DEL INSTRUMENTO XIFU DE LA MISION ATHENA. EN EL CAMPO CIENTIFICO, SE MAXIMIZA EL RETORNO CIENTIFICO DE LAS MISIONES INFRARROJAS Y DE RAYOS X PRESENTES Y SE PARTICIPA MUY ACTIVAMENTE EN LA PREPARACION DE UN AMBICIOSO PROGRAMA CIENTIFICO DE SPICA EN EL IR Y EN RAYOS X PARA ATHENA._x000D_ _x000D_ SE SOLICITA LA FINANCIACION PARA LOGRAR LOS SIGUIENTES OBJETIVOS CONCRETOS:_x000D_ A) ACTIVIDADES CIENTIFICAS Y TECNOLOGICAS EN SAFARI/SPICA, COMO CO-IP, PARA PREPARAR LA PROPUESTA DE SPICA A A LLAMADA M5 DE LA ESA._x000D_ ¿ DEFINIR LAS ESPECIFICACIONES TECNICAS Y REALIZAR EL DISEÑO OPTICO Y ESTRUCTURAL DEL NUEVO INSTRUMENTO SAFARI._x000D_ ¿ DESARROLLAR COMPONENTES CRITICOS Y TECNOLOGIAS HABILITADORAS EN IR, CREANDO Y CARACTERIZANDO DETECTORES DE VANGUARDIA PARA SAFARI Y MISIONES FUTURAS EN EL IR._x000D_ NOS CONCENTRAREMOS EN EL DESARROLLO DE DETECTORES SUPERCONDUCTORES Y DE GRAFENO DE ALTO RENDIMIENTO PARA EL RANGO 20-200 MICRAS._x000D_ _x000D_ B) DEFINIR LOS REQUERIMIENTOS Y REALIZAR EL ANALISIS MECANICO DEL CRIOSTATO DE XIFU APROVECHANDO LAS SINERGIAS CRIOGENICAS CON SAFARI (MISMO TIPO DE DETECTORES SUPERCONDUCTORES). _x000D_ _x000D_ C) CONTRIBUIR A LA FASE DE POST-OPERACIONES DE HERSCHEL CON LAS ACTIVIDADES YA INICIADAS EN LOS CENTROS DE CONTROL DEINSTRUMENTOS (ICCS), DESARROLLANDO Y MANTENIENDO HERRAMIENTAS DE ANALISIS Y _x000D_ REDUCCION DE CUBOS DE DATOS MOLECULARES (PAQUETE MADCUBAIJ, CAB)._x000D_ _x000D_ D) EXPLOTACION CIENTIFICA DE HERSCHEL, XMM-NEWTON Y CHANDRA, CON EL FIN DE QUE LOS EQUIPOS INVOLUCRADOS EN LOS CONSORCIOS CIENTIFICOS DE SAFARI Y XIFU PUEDAN LIDERAR PROGRAMAS QUE COMBINEN EL MODELADO DE DATOS IR Y DE RAYOS X EN EL ESTUDIO NUCLEOS ACTIVOS DE GALAXIAS Y DE ESTRELLAS MASIVAS EN LA VIA LACTEA Y EL GRUPO LOCAL._x000D_ _x000D_ E) EXPLOTACION MULTILONGITUD DE ONDA DE LOS DATOS DE HERSCHEL Y DE RAYOS X COMBINADOS CON PROGRAMAS DE FOLLOW UP CON OTROS INSTRUMENTOS. LOS PROXIMOS AÑOS SERAN FUNDAMENTALES PARA OBTENER RESULTADOS CIENTIFICOS SIN PRECEDENTES AL COMBINAR DATOS DE HERSCHEL, XMM Y CHANDRA CON OBSERVACIONES DE ALTA RESOLUCION ANGULAR DE ALMA, APEX, GTC, VLT Y HST. ESTA SINERGIA TAMBIEN PROMOVERA NUESTRO LIDERAZGO EN LA DEFINICION DE LOS PROGRAMAS CIENTIFICOS DE LA MISIONES SPICA Y ATHENA._x000D_ _x000D_ LA FINANCIACION QUE SE SOLICITA EN ESTE PROYECTO ES FUNDAMENTAL PARA LOGRAR EL RETO DE SER CO-IP DE SAFARI Y LIDERAR ASI LA EXPLOTACION CIENTIFICA DE DICHO INSTRUMENTO Y DE XIFU/ATHENA. (VER ACRONIMOS EN LA MEMORIA). (Spanish)
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In the last two decades, SPAIN has developed an important SCIENTIFIC AND TECHNICAL COMMUNITY IN INFRARROWING (IR) AND IN RATES X THAT WITH EXIT, AS CO-INVESTIGATOR, TO THE DEVELOPMENT AND SCIENTIFIC EXPLOTATION OF THE MAYORIA OF EUROPEAN SPACEMENTS._x000D_ _x000D_ The CAB sub-project Combines Expertise in CRIOGENIA TECHNOLOGY (A MK) and SPACIAL MECHANICAL WITH EXPERIENCE IN SCIENTIFIC EXPLOTATION IN MM/SUB/FAR-IR AND RAYS X, which would allow a QUANTITATIVE AND QUALITATIVE QUALITATIVE STATEMENT in SPANISH IN THE DESIGN AND DEVELOPMENT spatial INSTRUMENTATION IN these ENERGY RANGOs._x000D_ _x000D_ The challenge of continuating co-linear (mainly CO-INVESTIGATOR -CO-IP-) the development of the SAFARI cryogenic infrastructure in the future and away from the SPICAL mission and the development of sub-conductors is undertaken. IN THE CASE OF X-RAYS, THE CAB LEADS (MIGUEL PLUS IS XIFU CONSORTIUM BOARD MEMBER) THE DEFINITION AND CONSTRUCTION OF THE CHRYOSTAT OF THE XIFU INSTRUMENT OF THE ATHENA MISSION. In the SCIENTIFIC CAMP, the SCIENTIFIC RETORN OF Infrared AND RAYS X-Prepared Missions is maximised and very active in the PREPARATION OF AMBICIOUS SCIENTIFIC PROGRAMME OF SPICAL IN THE WORK AND IN RAYS X FOR ATHENA._x000D_ _x000D_ is requested to achieve the following CONCRETIVE OBJECTIVES:_x000D_A) SCIENTIFIC AND TECHNOLOGICAL ACTIVITIES IN SAFARI/SPICA, as CO-IP, to prepare the SPICAT PROPOSAL TO FALL M5 OF ESA._x000D_ DEFINING TECHNICAL SPECIFICATIONS AND RELATED DESIGNATIONS OPTIC AND STRUCTURAL OF THE NEW SAFARI INSTRUMENT._x000D_ DEVELOPMENTS CRITICAL COMPONENTS AND TECHNOLOGIES HABILITATORS IN IR, CREANING AND Characterising VANGUARDY DETECTORS FOR SAFARI AND FUTURE MISSIONS IN THE IR._x000D_ we agree on development of high-remuneration and high-remuneration GRAFENO DETECTORS for RANGO 20-200 MICRAS._x000D_ _x000D_ B) Define the requirements and carry out the mechanic analysis of the Xifu cryostat APROVECHANING CRIOGENIC SINERGIAS WITH SAFARI (MO TYPE OF SUPERCONDUCTOR DETECTORS). _x000D_ _x000D_ C) CONTRIBUTION TO THE HERSCHEL POST-OPERATIONS WITH ACTIVITIES AND INNICATION IN INstruMENT CONTROL CENTRES (ICCS), DEVELOPMENT AND MAINTENANING ANALISIS TOOLS AND _x000D_ REDUCTION OF MOLECULAR DATA CUBES (PAQUETE MADCUBAIJ, CAB)._x000D_ _x000D_ D) SCIENTIFIC EXPLOTATION OF HERSCHEL, XMM-NEWTON AND CHANDRA, with the end of which the EQUIPMENTS INVOLUCRED IN SCIENTIFIC CONSORCIES OF SAFARI AND Xifu CAN LIKE PROGRAMMS that combine the model of IR and RAYS X in the State active NUCLEOS OF GALAXIAS AND MASIVE STRELLS IN THE LACTEA VIA AND LOCAL GROUP._x000D_ _x000D_E) Multi-Length EXPLOTACTION OF HERSCHEL AND RAYS X DATAS Combined with FOLLOW UP PROGRAMMES WITH OTHER INSTRUMENTS. THE NEXT FEW YEARS WILL BE CRITICAL TO ACHIEVING UNPRECEDENTED SCIENTIFIC RESULTS BY COMBINING DATA FROM HERSCHEL, XMM AND CHANDRA WITH HIGH ANGULAR SOUL RESOLUTION OBSERVATIONS, APEX, GTC, VLT AND HST. This SINERGY will also promote our leadership in the definition of the scientific programmes of the SPICA and ATHENA mission._x000D_ _x000D__x000D_ THE FINANCIACTION that is requested in this project is a fundamental one to achieve the challenge of being co-IP of SAFARI and to lead the CIENTIFIC EXPLOTATION OF INSTRUMENT AND Xifu/ATHENA DICHO. (SEE ACRONMOS IN MEMORY). (English)
12 October 2021
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Torrejón de Ardoz
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Identifiers
ESP2015-65597-C4-1-R
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