PixeLearner: A Personalized ML-Powered App
Advanced Stellar Modeling
Sentiment Analysis on Movie Reviews using NLP and Machine Learning
Forecasting Stock prices using RNN
EnergyDash
PixeLearner was conceptualized with the primary intention of seamlessly integrating vision-based machine learning with the intricacies of natural language processing. The objective was clear - create a tool that offers a natural way to recognize and label individuals, thereby enhancing personal interactions.
The primary aim of PixeLearner is to seamlessly emulate human interactions - to spot familiar faces and instantly recall associated names, just as one would during a friendly meetup.
PixeLearner is more than just a project; it represents a step forward in how we interact with our environment. It's a testament to what can be achieved when vision and voice come together, and I'm excited about the path ahead. I am thinking to send the app for review. But before that there are a few minor things that need to polished. Thanks for reading and you can check the code on my github.
This project represents an intersection of state-of-the-art NLP techniques, statistical modeling, and advanced machine learning algorithms. Through meticulous design and implementation, a high-performance model was created to accurately classify movie reviews based on sentiment.
Data was sourced from the NLTK movie_reviews corpus and ingested through a comprehensive ETL pipeline using AWS Glue and Lambda functions, reflecting an efficient and scalable architecture.
Data preprocessing involved several complex steps, optimized for performance and accuracy:
Engineered a composite model combining Logistic Regression, Random Forest, Naive Bayes, and SVM with ensemble learning techniques. Utilized stochastic gradient descent for optimization, with a custom loss function defined by:
Implemented a robust training regimen with cross-validation and GridSearch for hyperparameter tuning. The models were evaluated using precision, recall, F1-score, and ROC-AUC metric, ensuring a well-balanced classification performance.
The SVM model achieved excellence with the highest ROC_AUC score. Insights drawn from this project are vital for areas like targeted marketing and user experience enhancement. Future directions involve integrating deep learning algorithms and experimenting with alternative vectorization strategies.
The goal of this project is to predict future foreign exchange rates using Recurrent Neural Networks (RNNs), a type of deep learning model well-suited for sequence prediction tasks.
The RNN architecture is designed to capture temporal dependencies in the data. The model is formulated as:
Here, \( h_t \) is the hidden state at time \( t \), \( x_t \) is the input at time \( t \), \( W \) represents weight matrices, and \( \sigma \) is the activation function.
Data preprocessing includes Min-Max scaling, expressed mathematically as:
The model demonstrated robust performance in predicting forex price movements. The predicted and actual prices closely followed each other, validating the model's accuracy. The use of an interactive Plotly graph allowed for an in-depth analysis of model predictions.
EnergyDash is an analytics platform designed to empower individuals to understand and optimize their household electricity consumption. Integrating real-time data via an API from power providers, it translates complex usage metrics into actionable insights.
The back-end of the application leverages AWS Lambda for serverless computation and Kinesis for real-time data streaming. A regression model built with Scikit-Learn analyzes consumption patterns, while the front-end visualization is constructed with Plotly.
EnergyDash provides a tailored user experience, enabling households to identify inefficiencies and take control of their energy spending. Through sophisticated analysis and user-friendly visualization, the platform contributes to sustainable living and cost savings.
This project involved the application of advanced computational techniques to simulate and analyze complex White Dwarf merger events. Utilizing the Magnetohydrodynamic (MHD) equations, the study extended the understanding of magnetized stellar interactions for precise astronomical modeling.
The simulation relies on the MHD equations, encompassing the conservation of mass, momentum, energy, and magnetic induction. These equations are expressed as:
\(\frac{\partial \rho}{\partial t} + \nabla \cdot (\rho \mathbf{v}) = 0\) (Conservation of Mass)
\(\frac{\partial \rho \mathbf{v}}{\partial t} + \nabla \cdot (\rho \mathbf{v} \mathbf{v} - \mathbf{B} \mathbf{B}) + \nabla p^* = 0\) (Momentum Conservation)
\(\frac{\partial E}{\partial t} + \nabla \cdot [(E + p^*) \mathbf{v} - \mathbf{B}(\mathbf{v} \cdot \mathbf{B})] = 0\) (Energy Conservation)
\(\frac{\partial \mathbf{B}}{\partial t} = \nabla \times (\mathbf{v} \times \mathbf{B})\) (Magnetic Induction)
Here, \(\rho\) is the density, \(\mathbf{v}\) the velocity, \(\mathbf{B}\) the magnetic field, and \(p^*\) the total pressure including magnetic contributions.
The simulations were conducted using the unsplit staggered mesh MHD solver in FLASH on the STAMPEDE 2 supercomputer. The project leveraged High-Performance Computing (HPC) for detailed analysis, facilitating comparison with traditional hydrodynamic models. This exploration enhances current astronomical understanding, offering novel insights into the intricate dynamics of stellar mergers.