Science

☁️ Modeling Development of Cloud Streets Over the Sahel

Since I'm only halfway through this project and it is ongoing, this is going to be short!

Introduction

This project investigates the development of cloud streets (long, parallel rows of cumulus clouds) over the Sahel, a region in Africa which lies underneath the Sahara. Specifically, we want to understand how soil moisture influences cloud formation and precipitation. This research is important because the Sahel is highly vulnerable to climate change. Improved understanding of rainfall patterns could directly benefit local communities, particularly those dependent on rain-fed agriculture. To address this question, we are looking at five simulations that vary in prescribed soil moisture levels.

Cloud streets photo
Figure 1: NASA image by Jeff Schmaltz, LANCE/EOSDIS Rapid Response.

Soil Moisture and the Surface Energy Budget

The surface energy budget (SEB) comprises five components: incoming shortwave (solar) radiation, outgoing longwave (surface and atmospheric) radiation, sensible heat flux (SHF), latent heat flux (LHF), and ground heat storage. Shortwave radiation warms the surface, which drives SHF (heating the near-surface air) and LHF (evaporation and moistening the air).

Soil moisture modulates the Bowen ratio, defined as SHF divided by LHF. This ratio critically affects two key heights: the lifting condensation level (LCL) and the planetary boundary layer (PBL) height. The PBL height rises with increasing SHF, promoting vertical lifting, while the LCL lowers with increasing LHF, enhancing moisture availability. For cloud formation to occur, the LCL must be at or below the PBL height.

SEB cycle
Figure 2: Surface energy budget diagram

Soil Moisture in Action

Highly saturated soil leads to stronger latent heat flux, as seen in the steeper dip in soil moisture content for the 100% saturation case compared to the 0% case. In a simulation like this, the LCL and PBL are both expected to be low which favors cloud formation! The next phase of our analysis will examine the resulting cloud formations alongside a calculation of the LCL and PBL heights across all five simulations to confirm this relationship.

Latent heat flux plot
Figure 3: Latent Heat Flux across different soil moisture levels

⚛️ Synthesis and Characterization of Lead-Free Halide Perovskites

My extended abstract for more depth!

Introduction

Halide perovskites are a family of materials making big waves in the science world for next-generation technology, including medical biosensing, light-emitting diodes (LEDs), and solar cells. Usually, these materials are lead-based. However, traditional lead-based perovskites face two major roadblocks: lead is super toxic, and the materials tend to degrade quickly when exposed to normal air and moisture.

To solve this, scientists are working to develop lead-free alternatives that are both environmentally friendly and stable. One method to supercharge these new materials is a process called "doping". Which is introducing tiny amounts of rare-earth elements, like Erbium (Er3+). These rare-earth elements act like internal light bulbs, producing incredibly sharp, predictable colors of light when energized.

This study investigates how Erbium doping changes the optical behavior of two lead-free materials: CAIC (Cs2AgInCl6) and CMBC (Cs4MnBi2Cl12). To see how well they fluoresce, we compared them to a classic lead-based benchmark material: KPC (KPb2Cl5).

Er-doped KPC, CMBC, and CAIC in ambient lighting vs UV
Figure 1: Er-doped KPC, CMBC, and CAIC in ambient light vs UV.

Goals and Methods:

The primary goals of this study were:

  1. Synthesize the Erbium-doped lead-free materials using a high pressure, hydrothermal method.
  2. Characterize exactly how these materials absorb and emit light using a spectrofluorometer.
  3. Compare our lead-free creations to the lead-based benchmark (KPC).

Hydrothermal Synthesis

To create these crystals, we used a hydrothermal method, which acts like an ultra-high-temperature pressure cooker to force high-quality crystal growth. This method involved:

  • Carefully weighing out precise precursor chemicals.
  • Placing the mixture into a tightly sealed, acid-resistant teflon vessel with 10 mL of hydrochloric acid (HCl).
  • Locking the vessel inside a stainless steel jacket and heating it in a furnace at 180°C (356°F) for 48 hours.
  • Safely cooling the mixture to room temperature, washing the brand-new crystal powders with ethanol, and drying them.
Autoclave/vessel setup
Figure 2: Teflon vessel and stainless steel jacket used for material synthesis.

Characterization Techniques

To analyze how our new crystals handle light, we placed them into a spectrofluorometer to perform:

  • Emission scans - Shining a fixed laser (like a UV or blue laser) at the sample to see what color it glows.
  • Excitation scans - Shifting through different wavelengths of light to find out exactly which energy level triggers the absolute brightest glow.

Results

Visible Fluorescence

Sample Name Base Perovskite Type Glow Color Under UV
Er: KPC Lead-Based Benchmark Vibrant Green
Er: CMBC Lead-Free Alternative Bright Orange
Er: CAIC Lead-Free Alternative None (Completely Dark)
Table 1: Fluorescence colors observed under UV excitation for each sample.

Both Er: CMBC and Er: KPC exhibited strong visible fluorescence under UV light, whereas Er: CAIC did not show significant emission. This suggests that the host material plays a critical role in the optical activity of Er3+ ions.

Excitation and Emission Spectroscopy

  • Er: KPC showed incredibly sharp, easily-identifiable peaks that align with the characteristics of Er3+ transitions.
  • Er: CMBC, however, presented broad energy bands. This tells us that the Manganese (Mn2+) is absorbing broad spectrum light and efficiently passing that energy off to our Erbium ions.

Sample Calculation: Er3+ Transition Energy

To verify the origin of the observed emission peaks, transition energies were calculated using the known electronic energy levels of Er3+ from a Dieke diagram.

Using the equation λ = 107 / ΔE allows for the wavelengths emitted/absorbed by different electron transitions. For example:

For the transition 4I15/24S3/2:

ΔE = Efinal - Einitial → 18500cm-1 - 0

So... ΔE = 18500cm-1

λ = 107 / 18500cm-1 = 540.5 nm

Emission and excitation spectrum graphs alongside energy transitions
Figure 3: Emission and excitation graphs alongside energy transitions. The blue arrows represent transitions shown.

Conclusions

  1. Success without Lead: The high-pressure hydrothermal method effectively cooks up brilliant, optically active crystals without needing toxic lead ingredients.
  2. The Host with the Most... Fluorescence: The choice of host material plays a huge role in the final performance. Multiple different colors can be achieved (or the light can be snuffed entirely) by swapping the structural host lattice.
  3. Direct vs. Hand-off Energy: Er:KPC displays direct excitation paths, whereas Er:CMBC relies on broad Mn2+ interactions to absorb light and pass it off to the Er3+.
  4. Customizable Tech: Because we can alter emission pathways and colors effortlessly, lead-free perovskites prove to be highly tunable and useful for future green tech, biophotonics, and future commercial lighting.
Ready Page 1 of 2