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NANO ALMA
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βWhat is?
The Atacama Large Millimeter/submillimeter Array (ALMA) is a radio telescope located in the Atacama Desert in Chile. It is one of the most advanced astronomical observatories in the world, comprised of 66 high-precision antennas that work together to observe the universe at millimeter and submillimeter wavelengths.
π§Components and Circuit
πLDR sensors
LDR1: ADC1 (GPIO 32)
LDR2: ADC2 (GPIO 33)
LDR3: ADC3 (GPIO 34)
LDR4: ADC4 (GPIO 35)
πDHT11 Humidity and Temperature Sensor
VDC: +3.3V GND: GND DATA (OUT): GPIO 2
πServo Motors
Servo1 (Vertical): Signal: GPIO 14 VCC: +5V GND: GND
Servo2 (Vertical): Signal: GPIO 15 VCC: +5V GND: GND
Servo3 (Horizontal): Signal: GPIO 16 VCC: +5V GND: GND
πYagi antenna Connected to the RTL-SDR dongle, which is connected to the laptop/PC
πPhotovoltaic Cell (5V, 1A) VCC: Connected to the input of the voltage regulator module GND: Connected to GND of the voltage regulator module
πVoltage Regulator Module Inpu
The Atacama Large Millimeter/submillimeter Array (ALMA) is a radio telescope located in the Atacama Desert in Chile. It is one of the most advanced astronomical observatories in the world, comprised of 66 high-precision antennas that work together to observe the universe at millimeter and submillimeter wavelengths.
π§Components and Circuit
πLDR sensors
LDR1: ADC1 (GPIO 32)
LDR2: ADC2 (GPIO 33)
LDR3: ADC3 (GPIO 34)
LDR4: ADC4 (GPIO 35)
πDHT11 Humidity and Temperature Sensor
VDC: +3.3V GND: GND DATA (OUT): GPIO 2
πServo Motors
Servo1 (Vertical): Signal: GPIO 14 VCC: +5V GND: GND
Servo2 (Vertical): Signal: GPIO 15 VCC: +5V GND: GND
Servo3 (Horizontal): Signal: GPIO 16 VCC: +5V GND: GND
πYagi antenna Connected to the RTL-SDR dongle, which is connected to the laptop/PC
πPhotovoltaic Cell (5V, 1A) VCC: Connected to the input of the voltage regulator module GND: Connected to GND of the voltage regulator module
πVoltage Regulator Module Inpu
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