Air Law and Kenya Civil Aviation Regulations
This domain tests the legal framework for instrument flight in Kenya: the ICAO standards adopted nationally, the Civil Aviation Act and KCAA regulations, licensing and recency, and the practical rules that govern IFR flight in Kenyan airspace.
Hierarchy of rules
The Chicago Convention and ICAO Annexes (notably Annex 1 licensing, Annex 2 rules of the air and Annex 11 ATS) are implemented in Kenya through the Civil Aviation Act 2013 and the Civil Aviation Regulations issued by the KCAA. The regulator also publishes AIP Kenya, AIRAC amendments and NOTAMs. For operational detail such as routes, minima and transition altitude, the current AIP is authoritative.
Licence and IFR obligations
An instrument rating permits flight under IFR in the aircraft categories endorsed. It depends on a valid licence, a Class 1 medical and English language proficiency. Before flight you must file an IFR flight plan, obtain and comply with an ATC clearance, make the required position reports and carry the fuel and alternate required by the regulations. Recency follows the KCAA licensing rules, including instrument experience and approach recency within the preceding 90 days; verify the current CARS rather than relying on memory.
Kenya airspace
Nairobi FIR (HKNA) is the main IFR environment. JKIA (HKJK), Wilson (HKNW), Mombasa (HKMO), Kisumu (HKKI) and Eldoret (HKEL) are the busiest aerodromes. Terrain forces a high transition altitude, published in AIP Kenya as 14,500 ft in the Nairobi FIR, with transition level normally FL150. QNH is reported in hectopascals.
Worked example
You are cleared into the Nairobi CTR at 9,500 ft. Because 9,500 ft is below the 14,500 ft transition altitude, the altimeter must be set to local QNH, not 1013.2 hPa. Only at or above the transition level do you fly standard pressure and report flight levels.
Marks-losing traps
Using QNE below the transition altitude; treating AIP as advisory; confusing ICAO Annex requirements with Kenyan variations; assuming radar coverage exists throughout the FIR.