Space Instrumentation Laboratory
A.Y. 2025/2026
Learning objectives
The course aims at developing the basic know-how in the field of space astrophysics instrumentation, with particular focus on active
and passive components used in radio and millimeter-wave astronomy.
During this module the students build and test a total power microwave receiver at 30 GHz. This receiver will be used to measure the
microwave radiation emitted by the Sun.
and passive components used in radio and millimeter-wave astronomy.
During this module the students build and test a total power microwave receiver at 30 GHz. This receiver will be used to measure the
microwave radiation emitted by the Sun.
Expected learning outcomes
At the end of the course the student will have acquired the following skills
·He/she will be able to calculate the expected signal observing a celestial source with a total power receiver coupled to a reflector
antenna
·He/she will be able to characterize the signal/noise properties of microwave components and of an integrated receiver with Vector
Network Analizer measurements
·He/she will be able to measure the noise temperature of a total power receiver
·He/she will be able to simulate the optical response of a feed-horn antenna coupled to a reflector antenna using the SRSR and
GRASP software
·He/she will be able to measure an antenna beam pattern by means of far-field measurements
·He/she will be able to measure the brightness temperature of a celestial source with a total power receiver coupled to a reflector
antenna
·He/she will be able to calculate the expected signal observing a celestial source with a total power receiver coupled to a reflector
antenna
·He/she will be able to characterize the signal/noise properties of microwave components and of an integrated receiver with Vector
Network Analizer measurements
·He/she will be able to measure the noise temperature of a total power receiver
·He/she will be able to simulate the optical response of a feed-horn antenna coupled to a reflector antenna using the SRSR and
GRASP software
·He/she will be able to measure an antenna beam pattern by means of far-field measurements
·He/she will be able to measure the brightness temperature of a celestial source with a total power receiver coupled to a reflector
antenna
Lesson period: Activity scheduled over several sessions (see Course syllabus and organization section for more detailed information).
Assessment methods: Esame
Assessment result: voto verbalizzato in trentesimi
Single course
This course cannot be attended as a single course. Please check our list of single courses to find the ones available for enrolment.
Course syllabus and organization
EDIZIONE PRIMO SEMESTRE
Responsible
Lesson period
First semester
FIS/05 - ASTRONOMY AND ASTROPHYSICS - University credits: 6
Laboratories: 48 hours
Lessons: 14 hours
Lessons: 14 hours
Professors:
Maino Davide, Mennella Aniello
EDIZIONE SECONDO SEMESTRE
Responsible
Lesson period
Second semester
FIS/05 - ASTRONOMY AND ASTROPHYSICS - University credits: 6
Laboratories: 48 hours
Lessons: 14 hours
Lessons: 14 hours
Professors:
Maino Davide, Mennella Aniello
Professor(s)