Role: Act as an expert academic presentation designer and a university-level mathematics student. Task: Create a professional, engaging, and well-structured PowerPoint presentation based on the initial project proposal provided below. The presentation is for a teacher/professor to review and approve my research topic on Probability Distributions and Random Variables. Design & Tone Guidelines: Keep the tone academic, formal, and confident. Do not overload the slides with text; use concise bullet points and bold keywords for readability. Include placeholders for mathematical equations (e.g., "[Insert characteristic function equation here]"). Suggest visual ideas for each slide (e.g., "Visual idea: A diagram of a satellite beaming a signal to Earth through noisy atmospheric layers"). Required Slide Structure (7-8 Slides): Slide 1: Title Slide (Project title, my name, date, course name) Slide 2: The Challenge of Deep Space Telemetry (Introduction & Context) Slide 3: The Core Problem (The problem statement regarding additive noise) Slide 4: Defining the Variables (Explain the true signal vs. noise using PMF and PDF) Slide 5: The Mathematical Solution (Explain how Characteristic Functions and MGFs solve the complex distribution problem) Slide 6: Signal Recovery (Explain Joint/Conditional distributions and Covariance) Slide 7: Expected Outcomes & Roadmap (What the project will deliver and the phase-by-phase plan) Slide 8: Conclusion & Q&A Source Material (Base the presentation entirely on this text): Research Topic: Deep Space Satellite Communication (Signal Processing) Project Title: Noise Deconvolution in Satellite Telemetry using Characteristic Functions Introduction and Context In modern aerospace engineering, transmitting data from deep-space satellites is highly complex. The final signal received by ground stations is heavily corrupted by independent sources of interference: cosmic radiation, atmospheric scattering, and thermal noise. We must utilize probability theory to model and filter this noise. Problem Statement How can we mathematically model and accurately recover a faint telemetry signal when it has been corrupted by the additive sum of multiple differently-distributed noise sources? Deriving its complex probability distribution manually is notoriously difficult. This project proposes using Characteristic Functions and Conditional Distributions to isolate the original signal. Mathematical Methodology Let true signal = S, cosmic noise = N1, atmospheric noise = N2. Received signal R = S + N1 + N2. Random Variables, PMF, and PDF: Signal S modeled as discrete RV (PMF). Noise N1, N2 modeled as continuous RVs (PDF). Characteristic Functions & Distribution Functions: To find the exact Distribution Function of R, we map to the frequency domain. The characteristic function of a sum of independent RVs is the product of their individual functions. MGF and Expectation: MGF computes the Mathematical Expectation E[R] and variance for signal-