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NASAPhoenix College
NASA ASCEND

Phoenix College NASA ASCEND / Spring 2025

Spring 2025
research record.

Original graphs for temperature, UV response and the modified radiation counter. Image-only graphs stay image-only: no invented points, smoothing or re-digitized curves.

Annotated burst altitude
87,885 ft
Spring 2025 counter figure
Profile maximum
≈ 63,000 ft
Altitude annotation; x-axis is time
UV measurements
Relative intensity
Independent source scales

Presentation figures are public. Original research documents, raw measurements, analysis files and source repositories are not provided as downloads.

Source-backed presentation

Read the actual evidence.

Every graph keeps its complete axes. Select a subject or enlarge a figure to read the labels. No smoothed replacement curves or invented observations.

Modified counter: Spring 2025. Complete source axes and plotted values.

Modified counter: Spring 2025

The legend reads 3/28/2025; the poster’s flight table reads 3/29/2025. It marks 87,885 ft burst and profile maxima near 63,000 ft. Horizontal: elapsed hours. Vertical: CPM.

Spring 2025 acquired-data report · original embedded figure 7. Original marks and axes retained.

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External temperature versus altitude. Complete source axes and plotted values.

External temperature versus altitude

The original profile is preserved. Narrative rounds the minimum to about −60 °C; the plotted curve extends below −60 °C. No precise minimum is inferred by digitizing the image.

Spring 2025 acquired-data report · original embedded figure 1. Original marks and axes retained.

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UVA graph: altitude in feet on the horizontal axis and relative intensity on the vertical axis.

UVA relative intensity versus altitude

Horizontal: altitude in feet. Vertical: relative intensity. The broad range at each altitude is preserved, rather than replaced by a smooth trend. UVA uses its own intensity scale; these values are not established here as calibrated irradiance.

Spring 2025 acquired-data report · original embedded figure 2. Original marks and axes retained.

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UVB graph: altitude in feet on the horizontal axis and relative intensity on the vertical axis.

UVB relative intensity versus altitude

Horizontal: altitude in feet. Vertical: relative intensity. Read the UVB scale separately from UVA: a taller plotted trace is not automatically a larger physical irradiance when the axes use different ranges.

Spring 2025 acquired-data report · original embedded figure 3. Original marks and axes retained.

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UVC graph: altitude in feet on the horizontal axis and relative intensity on the vertical axis.

UVC relative intensity versus altitude

Horizontal: altitude in feet. Vertical: relative intensity. UVC uses its own scale. This is the recorded channel response, not independently calibrated ambient UVC exposure; sensor spectral response and calibration must be checked before making that claim.

Spring 2025 acquired-data report · original embedded figure 4. Original marks and axes retained.

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Student neutron-detection concept. Complete source axes and plotted values.

Student neutron-detection concept

Published schematic of the team’s modified-counter experiment. Counts are not calibrated neutron-only flux or dose, and this diagram does not quantitatively establish shielding performance.

Spring 2025 acquired-data report · original embedded figure 5. Original marks and axes retained.

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Source notes that matter.

Source: team-supplied “Spring 2025 launch acquired data” report and photographed presentation boards. Student research, not independent instrument certification. Detector counts are not dose; channel output is not automatically calibrated concentration or irradiance.

Scientific context: NASA atmospheric radiation research · NOAA ultraviolet radiation background. Context does not validate these instruments.